The galaxy presents as a well-defined, flattened spheroid. The color profile indicates a dominant yellow-orange central bulge region, potentially indicating an older stellar population in this area. Fainter bluish light is observed in the outer regions, suggestive of possible younger stars there. The galaxy is relatively smooth in appearance, with no clearly defined spiral arm structure or other features. There is a slight asymmetry to the galaxy, with one side appearing more extended than the other. No evidence of active galactic nuclei or significant dust lanes is apparent in the image. Based on the overall morphology and color distribution, the galaxy is likely an early-type spiral or lenticular galaxy.
