The galaxy appears to be a relatively compact object. It exhibits a subtle disk-like structure, though this is not highly prominent. The color profile suggests a mix of stellar populations. There is a smooth, centralized component, possibly a bulge, which appears redder in color indicating older stars and or dust absorption. Fainter blue regions are apparent, hinting at potential star forming regions. There are some faint features and disturbances, suggesting that it may be in the process of merging with a smaller galaxy. These features could also be the result of tidal interactions with nearby galaxies, or an indication of minor interactions in the recent past. Overall, the galaxy presents a somewhat disturbed morphology.
