The galaxy appears to be an elliptical type, characterized by its generally smooth and featureless morphology. There is no visible spiral arm structure or prominent dust lanes. The galaxy exhibits a centrally concentrated luminosity profile, with the core being significantly brighter and more concentrated than the outer regions.

The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue of the central region. There is a hint of bluer light in the outer regions, potentially indicating some ongoing or recent star formation at a lower rate. The galaxy exhibits a roughly circular shape. There is no visible evidence of a recent or ongoing major merger event. The object appears relatively isolated, with no obvious tidal features or close companion galaxies visible in this image.
