The galaxy appears to be an elliptical galaxy, presenting a smooth, mostly featureless morphology. It exhibits a somewhat round shape, with a slight elongation, possibly tending toward a lenticular classification. The central region displays a bright, concentrated luminosity, indicative of a substantial stellar population. There is a color gradient, shifting from yellowish at the core toward redder hues in the outer regions. No prominent spiral arms or dust lanes are visible. Overall, this galaxy seems to be a fairly evolved system, likely with a relatively low rate of current star formation activity. There is no evidence of significant tidal disturbances or ongoing merger activity.
