The galaxy presents as a centrally concentrated, luminous object with a relatively smooth appearance. The core exhibits a yellowish hue, suggesting a population of older stars. There appears to be a slight extension or plume extending from the main body of the galaxy towards the upper right, potentially indicating tidal interaction or a minor merger event. The galaxy lacks discernible spiral arm structures or prominent dust lanes, suggesting it could be an elliptical galaxy or a lenticular galaxy with a weak disk. Overall, the light distribution appears relatively uniform, with the majority of light emanating from the central region. Subtle irregularities in the outer regions hint at past or ongoing gravitational disturbances. The overall color suggests moderate star formation.
