The galaxy presents as an elliptical morphology, exhibiting a generally smooth, symmetrical light distribution. There is a slight elongation to its shape, appearing more "in between" round and cigar-shaped. The galaxy exhibits a brighter, condensed central region which is likely its bulge. It displays a generally blue hue, suggesting some ongoing star formation, albeit possibly at a low rate. No obvious spiral arm structures are present, nor is there any strong evidence of tidal features, major mergers or strong morphological disturbances in the immediate vicinity. The overall structure seems relatively undisturbed, with only minor disturbances to the galaxy's shape.
