The galaxy presents as a single, concentrated object, roughly elliptical in shape. It appears to be dominated by an older stellar population, implied by the yellowish-orange hue concentrated towards the galaxy's center. Fainter, bluer regions are visible in the outer parts of the galaxy, suggesting the presence of some younger stars or ongoing star formation activity, though at a low rate. There is a slight hint of a disk-like structure. No major mergers or tidal disturbances are apparent in the image, although there are some minor disturbances present.
