The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. There is a general lack of discernible spiral arm structure or prominent dust lanes. The galaxy exhibits a noticeable color gradient, appearing more yellow-orange towards the center, suggesting a higher concentration of older stellar populations in the nuclear region. The outer regions appear slightly bluer, indicative of a younger stellar population, although this is not particularly pronounced. There is no obvious active galactic nucleus or evidence of ongoing major mergers. It appears to be an isolated galaxy with no nearby interacting companions visible in the image.
