The galaxy appears as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution suggests a dominant bulge component, evidenced by the smooth transition in brightness from the core outwards. There is no obvious spiral arm structure or strong dust lane visible. The core is bright and yellowish-white suggesting a population of older stars. The outer regions become fainter and slightly redder in color, potentially indicating a slightly younger stellar population, however it could also be a result of dust extinction. The overall impression is of a mature, early-type galaxy with a substantial spheroidal component. There is a slight elongation visible in the galaxy's shape, which is likely a true feature. There are no obvious signs of recent major merger activity, such as tidal tails or strong morphological disturbances.
