The galaxy presents as a somewhat elliptical morphology, displaying a smooth overall appearance. A distinct central bulge region is observed with a concentrated, bright yellow color, suggesting a high density of older stellar populations. The outer regions of the galaxy show a fainter, bluer color, possibly indicating the presence of younger stars and ongoing star formation, although the smoothness of the galaxy suggests that star formation is relatively diffuse. There is a very slight suggestion of spiral arm structure, but it is not highly pronounced. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There may be a minor disturbance or irregularity in the morphology. The size of the galaxy appears typical for a spiral galaxy. The galaxy has a moderately high mass, typical of massive disk galaxies. The rate of star formation is relatively high.
