The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its color appears distinctly red, suggesting a population dominated by older stars and a lack of significant ongoing star formation. The galaxy appears quite round, lacking any obvious strong tidal features or morphological disturbances indicative of recent major merger activity, though there might be a very slight asymmetry. There is a suggestion of multiple cores or possible interaction but the resolution of the image is not high enough to determine. The galaxy exhibits a compact morphology and the light is concentrated towards its center. Overall, this galaxy appears to be a massive and evolved system, with a high degree of central concentration and a smooth stellar distribution.
