The galaxy presents as a largely elliptical structure with a smooth, concentrated luminosity profile, suggesting a classification towards early-type morphology. The dominant feature is a bright, centrally located core. There is a noticeable decrease in luminosity moving from the core outwards, with an apparent lack of significant spiral arm structures. There are some minor irregularities along the outskirts of the galaxy. The galaxy has a general yellowish-white hue, which indicates that it is comprised mostly of older stars. This color is more prevalent toward the central bulge, with slight bluer regions in the outskirts. The shape is mostly circular, with some slight elongation. No obvious signs of ongoing major merging events or significant tidal disturbances are apparent in this image, but some subtle minor interactions cannot be ruled out.
