The galaxy presents as a primarily smooth, elliptical morphology. The central region exhibits a bright core, possibly indicative of an active galactic nucleus or a high concentration of older stars. The galaxy appears generally round with a slight extension in shape. There is no clear evidence of spiral arm structures or significant dust lanes. The overall color gradient suggests a stellar population dominated by older, redder stars, although some bluer tones are present in the outer regions. The disk appears relatively undisturbed with no major merger activity currently disrupting its structure. There is no apparent interaction with neighboring galaxies. Overall, the galaxy exhibits characteristics consistent with a relatively evolved, quiescent system with ongoing, yet moderate, star formation.
