The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a somewhat elongated shape, leaning towards cigar-shaped rather than perfectly round. There is a noticeable color gradient, with the central region displaying a brighter, whiter hue, possibly indicating a higher concentration of older stars. The outer regions show hints of bluer tones, which might suggest some recent star formation, although the overall rate appears to be relatively low. There are some minor indications of disturbances or asymmetries in the outer regions, which may be the result of a minor interaction. No spiral arms are visible.
