The galaxy presents as a slightly elongated, diffuse object. Its core region is noticeably brighter and appears nearly spheroidal, exhibiting a smooth luminosity profile that gradually decreases outward. There is a faint, extended halo surrounding the core. The overall color appears to be moderately blue, suggesting some ongoing star formation, although the light is dominated by older stellar populations. No distinct spiral arms or bar structures are visible. The morphology is consistent with an elliptical galaxy, possibly of type E3-E5 given the slight ellipticity. There is evidence of minor tidal disturbance or interaction, potentially from a past merger event.
