The galaxy presents as a somewhat elliptical, smooth object with a concentrated central bulge. There is a noticeable color gradient within the galaxy, shifting from a yellower hue in the core to a slightly bluer color in the outer regions. There's no visible evidence of spiral arm structure or significant dust lanes. The overall impression is of a galaxy that is relatively evolved, likely with a substantial population of older stars and a considerable stellar mass. There may be subtle distortions or irregularities in the outer regions, possibly indicating past or ongoing interactions with smaller galaxies, but these are not overtly prominent. The light distribution appears relatively uniform, lacking bright knots or other high-contrast features that would suggest intense star formation regions.
