The galaxy presents as a moderately bright, roughly elliptical object. There is a strong central concentration of light, suggestive of a prominent nucleus or bulge. Moving outward from the center, the light fades gradually, with no sharp cutoff in luminosity. Faint, diffuse extensions are possibly visible, although they are not well-defined. There may be some indication of minor disturbances or tidal features, as the outer regions of the galaxy appear slightly asymmetrical. The overall color suggests the galaxy is composed of a population of stars spanning a range of ages, though the light may be dominated by older stars. There is little indication of active star formation, and a smooth structure indicates that the galaxy is likely an elliptical galaxy.
