The galaxy presents as a moderately bright, compact object with a relatively smooth morphology. It appears largely featureless in the observed optical bands, lacking prominent spiral arms or a distinct bar structure. The shape is more elliptical than circular, tending towards an 'in-between' or transitional form. The central region exhibits a slightly higher surface brightness, suggesting a concentration of stars or a small bulge component.

There is no obvious sign of ongoing major mergers or tidal disturbances, although some minor irregularities in the outer regions might indicate past interaction or internal activity. Color gradients across the galaxy are subtle, with a tendency towards redder colors in the central region and slightly bluer colors in the outskirts, which is consistent with a decreasing age of the stellar populations from the center to the outer regions. The overall color suggests a substantial population of evolved stars.
