The galaxy presents as a largely featureless elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The core region exhibits a bright, nearly uniform yellowish color suggesting an older stellar population. There is no apparent spiral arm structure or dust lane obscuration. Faint, diffuse light extends outwards from the core, gradually fading into the background sky. The overall shape approximates a slightly elongated spheroid. There is no evidence of tidal disturbances or ongoing major merging activity in this image. The galaxy appears to be relatively isolated, and undisturbed.
