This galaxy presents as a generally smooth, elliptical form, though not perfectly round. It displays a slightly elongated shape, deviating slightly from a perfect sphere. The central region exhibits a brighter concentration of light, suggestive of a dense galactic nucleus. Moving outwards, the luminosity gradually decreases. There are faint, somewhat irregular features or disturbances extending from the main body of the galaxy that may be a result of a minor gravitational interaction with a smaller object. Based on the overall red color and smoothness, this is likely an older galaxy comprised mainly of older stars.