The galaxy presents as a somewhat elliptical, rather smooth-appearing structure. Its core exhibits a concentrated, bright luminosity with a dominant orange-red hue, suggesting an older stellar population within the nucleus. The outer regions display a faint blue-green tint. A slight elongation is observed, suggestive of a disk-like component or tidal interaction. The overall morphology indicates a system undergoing limited active star formation, with a substantial fraction of its stellar population likely in a post-starburst phase. There is no evidence of strong tidal features or major mergers. The galaxy appears to be relatively isolated, without any obvious nearby companions or significant disturbances.
