The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, bright central bulge that gradually fades into a more diffuse halo. The color profile suggests a population of older stars, as indicated by the yellowish-orange hue dominating the central region. There is little evidence of prominent spiral arms or dust lanes. The overall shape is predominantly round, with no apparent signs of significant tidal disturbances or ongoing major mergers. Minor asymmetries are undetectable at this resolution. The galaxy's structure indicates it is likely a mature system with a well-established stellar population and limited recent star formation activity.
