The galaxy presents as a relatively smooth and centrally concentrated object. The core exhibits a bright, golden-yellow hue, suggesting an older stellar population. The overall morphology appears elliptical, with no discernible spiral arm structure or prominent disk features. The light profile fades smoothly outwards from the core. There may be some very faint, subtle, asymmetric extensions of the light distribution, but these are difficult to resolve clearly and do not suggest a major ongoing merger. The color gradient suggests a centrally concentrated population of older stars with ongoing, but likely slow, star formation.
