The galaxy presents a predominantly smooth morphology, with a slightly elongated, cigar-like shape. The light distribution suggests a bulge-dominated system, possibly an elliptical galaxy or a lenticular galaxy with a significant bulge component. There are indications of a central, bright region, presumably the galactic nucleus. The galaxy exhibits a color gradient, shifting from a more reddish hue in the central region to a somewhat bluer tint towards the outer edges of the disk. There is no evident spiral arm structure or signs of recent major mergers. The lack of pronounced features suggests a relatively quiescent star formation history, although some low levels of star formation may be occurring. Minor asymmetry in the outer regions may be present, hinting at potential past interactions or minor disturbances, but overall, the galaxy appears relatively undisturbed.
