The galaxy presents as a somewhat elliptical, moderately luminous object. It appears to be relatively compact, with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions display a slightly bluer tint, possibly indicating some ongoing star formation, though at a relatively low rate. There is a subtle suggestion of a disk-like structure, but it's not prominently defined; the galaxy generally seems to be lacking distinct spiral arms or other pronounced features. There is a mild indication of possible minor disturbances or interactions with other bodies but it does not show clear signs of an active merging event, or a major disruption of its structure.
