The galaxy presents as a largely smooth and relatively round structure. There is a concentration of light toward the center, suggesting a prominent bulge component. The outer regions exhibit a fainter, more diffuse halo. Based on the red color, the galaxy is likely composed of an older stellar population. There are no readily apparent spiral arms or strong dust lanes, suggesting a galaxy with minimal ongoing star formation. Indications of any major mergers or significant tidal disturbances are absent. There may be minor disturbances, but any merging is minor if happening. Overall, the galaxy appears to be an elliptical type, generally featureless in appearance.
