The galaxy presents as a relatively smooth, centrally concentrated object. There is a distinct core region exhibiting a yellowish hue, suggesting a population of older stars. The outer regions appear less concentrated, with a subtle red shift. The overall shape is roughly elliptical, with a hint of elongation, though it trends toward a more circular form. There is no clear evidence of spiral arms, a prominent disk, or ongoing major mergers. Subtle irregularities are present, hinting at possible minor disturbances or past interactions. The light distribution fades gradually from the central core outward.
