The galaxy presents as a somewhat amorphous structure with a concentrated central region. The light distribution suggests an elliptical morphology, with an absence of prominent spiral arms or a well-defined disk. The galaxy exhibits a reddish-yellow hue, suggestive of an older stellar population and a low rate of on-going star formation. The lack of distinct blue regions or HII emission indicates limited recent or current star birth activity. Faint extensions or tidal features are not readily apparent in this image, suggesting that if the galaxy is involved in a merger, it is most likely a late-stage merger, or has been involved in a merger in the distant past. The galaxy appears relatively smooth in texture, without significant internal substructure visible at this resolution.
