The galaxy presents as a roughly elliptical, though not perfectly round, extended light source. A central, brighter core region is apparent, suggestive of a concentrated nucleus. Moving outwards from this core, there is a gradual decrease in luminosity. The galaxy exhibits a relatively smooth appearance overall, but there are hints of some structure or features, particularly in the outer regions, where a slight asymmetry or faint extension might be present. The color gradient indicates a higher concentration of older stellar populations within the central regions, with potentially some bluer, younger stars or star-forming regions in the outer disk. No obvious spiral arms are visible, but the presence of some faint features suggests the possibility of underlying disk structures or past merger events causing minor disturbances. Overall, this galaxy appears to be a fairly massive system with a relatively low specific star formation rate, indicating that star formation is not rampant but still occurring. There is no obvious indication of any ongoing major merging events.
