The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears uniform, lacking any distinct spiral arm features. The core exhibits a bright, yellowish hue, potentially indicative of an older stellar population. The overall color gradient suggests a transition to redder hues towards the outer regions, possibly implying a decline in recent star formation activity in these areas. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The morphology appears generally relaxed and symmetrical.
