The galaxy presents as a somewhat elliptical, moderately luminous object. Its central region exhibits a bright, concentrated core, suggesting a significant concentration of older stars. The overall color profile leans toward the redder end of the spectrum, further indicative of an older stellar population and relatively low levels of ongoing star formation. There is a smooth, diffuse outer halo extending beyond the bright central bulge, and subtle disturbances in the form of slight asymmetries are possibly present. No distinct spiral arm structures are discernible. The object appears relatively isolated, with no clear evidence of major ongoing merging activity, although subtle disturbances or tidal features might indicate past or minor interactions. The morphology is largely consistent with an early-type galaxy transitioning from disk-dominated to more spheroidal systems.
