The galaxy presents an elliptical morphology, with a notable bulge. There is asymmetry within the galactic structure, with what seems to be an extension or possible tidal feature on one side, indicating potential past or ongoing interaction. The color distribution appears to be dominated by redder hues in the central region, possibly indicative of an older stellar population and/or dust obscuration. The outer regions show some bluer colors. The structure appears relatively concentrated, lacking strong spiral arm features and indicative of Sersic profile.
