The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light profile appears relatively featureless, lacking prominent spiral arms or distinct dust lanes. The shape is somewhere between a perfect circle and a cigar, appearing somewhat elliptical, though it is mostly round.

There is a distinct central bulge that dominates the galaxy's light output. The bulge displays a yellowish-white hue, possibly indicating an older stellar population. The outer regions of the galaxy show a bluer tint, which might be indicative of some ongoing star formation, though it seems minimal. There is a possible minor disturbance on one side, and a hint of faint, diffuse outer structure, but it is difficult to discern detail. The galaxy appears relatively isolated, without obvious signs of a major merger event.
