The galaxy presents as a moderately luminous, spatially extended object. It exhibits an overall smooth morphology, with a centrally concentrated, roughly ellipsoidal light distribution. The core region appears yellowish, indicative of a potentially older stellar population dominating the central mass distribution. Moving outwards from the core, the colors transition toward a slightly bluer hue. The overall shape is elliptical rather than spiral, with no strong evidence of spiral arm structures. The galaxy does not appear to be undergoing any major ongoing mergers, though the slight asymmetry in the outer regions could suggest minor disturbances. It is likely a large and relatively massive galaxy, with moderate levels of star formation.