The galaxy presents as a largely featureless, elliptical morphology. Its core exhibits a concentrated, bright, yellowish-orange hue, suggesting a population dominated by older stars and potentially a significant dust component. There is little evidence of spiral arm structure or significant star formation regions. The overall shape appears close to circular, with no discernible elongation or tidal distortions. A faint, diffuse halo surrounds the central core, gradually fading into the background sky. There is no indication of a major ongoing merger, although minor disturbances can not be ruled out at this resolution.
