The galaxy appears to be a relatively small, elongated object, likely an elliptical galaxy viewed at an angle. Its central region exhibits a diffuse glow, suggesting a concentration of older stars. Proceeding outward, the light gradually diminishes, blurring into the background sky. There is little evidence of spiral arms or significant star formation, as suggested by the lack of prominent blue regions. Its shape appears cigar-like, with no obvious disk structure visible. Overall, the galaxy presents a smooth appearance with a relatively uniform color profile, suggestive of an older stellar population and minimal ongoing star formation. There is no visible evidence of merging or tidal disturbances.
