The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears uniform, lacking any significant spiral arm features or prominent dust lanes. The color gradient suggests a population of older stars dominating the galaxy's composition, trending towards redder hues. The shape is largely spheroidal, with a slight deviation towards an elliptical form. There is no apparent evidence of ongoing major merger activity or significant tidal distortions. Small color variations may be evidence of some star formation.
