This galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. The system appears to consist of two primary components: a dominant, seemingly spheroidal body and a less distinct, bluish extension.

The main component is characterized by a relatively smooth, concentrated light distribution. It is somewhat ellipsoidal in shape, leaning towards the rounder end of the spectrum. The dominant coloration is yellowish-orange, suggesting an older stellar population.

Extending from the primary body is a diffuse, less concentrated region of bluish light. This area shows some irregularities, possibly distorted tidal features resulting from gravitational interaction. The blue color suggests the presence of younger, hotter stars likely formed through stimulated star formation.

The overall structure is indicative of a galaxy undergoing a merger, where gravitational forces are actively reshaping the stellar distribution and potentially triggering new episodes of star formation. A significant portion of the galaxy's light appears concentrated in the main body, while the disturbed region displays a distinct stellar population.
