The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with minimal discernible substructure. The object's shape is somewhat elongated, trending towards a moderate ellipticity. A prominent central bulge is visible, with a concentration of light intensity, gradually decreasing towards the outer regions. Color gradients are apparent within the galaxy; the core region displays a yellowish-white hue, suggesting a population of older stars. The outer regions exhibit a faint, diffuse greenish tint, potentially indicative of ongoing, albeit low-level, star formation. No clear spiral arm structures or dust lanes are observed. The galaxy appears isolated, showing no obvious signs of tidal interactions or merging events with neighboring galaxies.
