The galaxy presents a largely smooth morphology, exhibiting a concentrated central bulge and a relatively faint, diffuse surrounding halo. It appears elliptical in shape, nearly circular with a small degree of elongation. Its color index suggests a population of older stars, with light trending towards the redder end of the spectrum. There's no discernible spiral arm structure or significant dust lane visible. The galaxy appears relatively undisturbed, showing no obvious signs of a major merger event or strong tidal interactions. There might be very minor asymmetry in the outer regions. The galaxy has a calculated redshift suggesting that the galaxy is receding away from us. The brightness indicates that it is a fairly luminous object, suggestive of a large mass and high number of stars.
