The galaxy presents a generally elliptical morphology. The core region exhibits high luminosity, appearing nearly spherical and featureless. This bright central area fades into a more diffuse halo, extending outwards. The halo appears relatively smooth with no distinct spiral arm structures visible. The galaxy’s color profile suggests a population of older stars and a lack of significant dust lanes or active star formation regions. The overall impression is that of a galaxy with a substantial spheroidal component. There are no visible signs of recent major mergers or significant tidal disturbances. The light appears to be dominated by the redder end of the spectrum.
