The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated, bright central bulge is apparent, which gently diffuses outwards into a less defined halo. The galaxy exhibits a slight elongation; its shape can be best described as somewhere between perfectly round and cigar-shaped. There are no distinct spiral arms, bar features, or obvious signs of ongoing mergers or major disturbances to its overall morphology. The color profile appears to be overall redder in the central region, grading to a bluer hue at the edges, suggestive of a higher population of older stars in the core and relatively younger populations in the outskirts. It looks like star formation is low.
