This galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. Two distinct components are visible.

The primary component presents a relatively smooth, elliptical appearance with a concentration of light towards the core. The color profile indicates a mixed population of stars, appearing somewhat redder overall, with the presence of a central blue region suggesting possible ongoing star formation there.

The secondary component, positioned adjacent to the primary, displays a more irregular shape and a distinct orange-red hue. This color suggests an older stellar population, possibly dust-obscured, or could represent tidal debris resulting from the interaction.

A faint bridge of material appears to connect the two components, indicating gravitational interaction. The overall system displays evidence of disturbance, likely attributed to the merging process.
