The galaxy appears as a moderately sized, lenticular or early-type spiral. It exhibits a smooth, centrally concentrated luminosity profile, indicative of an evolved stellar population. The color gradient suggests a redder core region, potentially populated by older stars, with a subtle blueish hue emerging in the outer disk, hinting at some recent, low-level star formation activity. There is no apparent spiral arm structure or significant dust lane features visible in the image. The overall morphology is more elongated than circular, leaning towards an elliptical shape, but it does have a clear, distinct disk-like structure with a central bulge. There is no evidence of any major mergers or significant tidal disturbances. The general appearance is of a well-ordered, mature galaxy undergoing minimal current star formation.
