The galaxy presents a somewhat elliptical morphology, appearing more cigar-shaped than circular. The core region is relatively bright and exhibits a yellowish hue, suggesting a population of older stars. A fainter, bluer disk-like structure is visible extending outward from the central bulge, albeit with lower surface brightness. This bluer light implies the presence of some younger, hotter stars, suggesting ongoing or recent star formation, although at a comparatively low rate. There is little evidence of strong spiral arm structure or significant tidal disturbances; the galaxy appears generally smooth and undisturbed. Overall, the galaxy appears to be an intermediate-mass system undergoing a relatively quiescent phase of stellar evolution.
