The galaxy presents as a smooth, elongated structure, likely a lenticular or elliptical galaxy viewed from an oblique angle. It exhibits a concentration of light towards the center, suggesting a prominent galactic nucleus. The color appears to be relatively uniform across the galaxy's body, with a reddish hue indicative of an older stellar population and lower ongoing star formation. There is a lack of distinct spiral arm structure or prominent dust lanes, further supporting its classification as a smooth, early-type galaxy. The overall morphology suggests a system nearing the end of its star-forming lifecycle, with a dominant population of older, redder stars. There are no obvious signs of recent or ongoing mergers or tidal interactions.
