The galaxy presents as a luminous, centrally concentrated object with a generally smooth appearance. There is evidence of a faint disk-like structure. The central region exhibits a bright, unresolved core, suggesting the presence of a substantial bulge. Some degree of disturbance is present and a potential merger. The galaxy's overall shape is elliptical-like with a slight elongation. The color profile is consistent with an evolved stellar population, with a dominance of redder wavelengths relative to bluer ones, particularly in the central bulge. The galaxy does not exhibit prominent spiral arms or significant dust lanes.
