This galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated luminosity gradient, indicative of a spheroidal component, possibly a bulge. The galaxy appears slightly elongated, with the light distribution exhibiting an intermediate degree of ellipticity. There is a subtle color gradient, with the core appearing more yellow and the outer regions exhibiting a bluer hue, possibly indicating younger stellar populations further from the core. There may be minor asymmetry present, but no evidence of significant tidal disturbances or ongoing mergers is apparent. Based on the morphology and color, it appears to be an evolved system with a dominant older stellar population.
