The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually decreases in intensity towards the outer regions. There is no clear evidence of spiral arm structure or a distinct galactic disk. The galaxy appears to be relatively isolated, lacking any significant signs of tidal interactions or ongoing mergers. The color suggests a population dominated by older stars, indicative of a relatively low star formation rate.
