The galaxy presents a largely smooth morphology, suggesting an elliptical or lenticular classification. The light distribution is centrally concentrated, exhibiting a gradual decline in surface brightness with increasing radius. The core is a bright yellow-white hue, with the yellow suggesting a population of older stars. Moving outward, the colour shifts towards a redder hue, implying the presence of cooler, aging stellar populations in the outer regions. There is no discernible spiral structure or prominent dust lanes. The overall shape appears roughly ellipsoidal. Subtle irregularities are observed, suggesting a possibility of a past minor merger event or tidal interaction. There does not appear to be any ongoing major merging. The lack of distinct features and the smooth, centrally concentrated light profile are consistent with a relatively evolved system, with suppressed recent star formation.
