The galaxy presents as a moderately luminous, elliptical system. Its core appears bright and concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population dominated by evolved stars. Extending outward from the core, a fainter, more diffuse halo is observed. This outer region displays a subtle bluish tint, hinting at the presence of some younger, hotter stars and potential ongoing star formation. The overall shape of the galaxy is somewhat elongated, deviating slightly from a perfect circular form, though without any clear signs of a major merger event or strong tidal disturbances. There are some subtle irregular features, perhaps indicating minor interactions or internal dynamics. Based on its color profile and morphology, this galaxy is likely a relatively massive system with a mix of stellar populations and a moderate rate of star formation.
