The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely rounded, with only a subtle deviation from perfect circularity. The light profile suggests a relatively homogenous stellar population with a possible bulge, lacking any distinct spiral arm structures or bars.

The galaxy’s color gradient transitions from a warmer, yellower core to cooler, bluer outer regions. This suggests a potential difference in stellar ages or metallicities, with the central bulge possibly hosting an older, redder stellar population, while the outer regions may contain younger, bluer stars. There is no significant evidence of ongoing major mergers or tidal disturbances, although some slight asymmetries in the outer regions could imply minor past interactions. There may be a low level of star formation in the galaxy.
