The galaxy presents as a roughly elliptical structure with a noticeable bulge. There is an apparent flattening suggesting a possible disk component, but this is not highly pronounced and the galaxy leans more to being spheroidal than a spiral. It appears fairly well-defined. There are color gradients across the galaxy, with the central region appearing more red/yellow and the outer regions exhibiting a slight bluish tinge which could indicate areas of active, but not very high, star formation in the outer disk and a population of older stars concentrated in the bulge. There are no clear indications of prominent spiral arms or bar structure, nor are there obvious signs of ongoing major mergers or tidal disturbances, although very faint signs of minor disturbance cannot be ruled out. Overall, the galaxy seems to be a fairly undisturbed system with moderate mass.
