The galaxy presents as a somewhat blended system, exhibiting characteristics of both an elliptical galaxy and a potential merging event. The dominant, central component displays a smooth, concentrated luminosity profile, suggestive of an elliptical galaxy. This central region emits primarily in the redder bands of the spectrum, indicating an older stellar population, with only modest on-going star formation.

A secondary, bluer component is observed adjacent to the central region. This area of bluer light suggests the presence of younger, hotter stars, and potentially an ongoing star forming region. Morphologically, the system displays signs of disturbance. Based on the irregular shape and dual component nature, the galaxy is likely undergoing or has recently undergone a merger. A small tidal tail or bridge may be present, indicative of gravitational interaction.
