The galaxy appears as a relatively smooth, elliptical-like object with a high degree of central concentration. Its color suggests a population of older stars, predominantly emitting in the redder wavelengths. The galaxy presents a predominantly featureless morphology, lacking clear spiral arms or a pronounced disk structure. The main body of the galaxy appears generally rounded in shape. There is a faint, diffuse halo surrounding the central region, which is more concentrated. There is no readily apparent evidence of ongoing major merger activity or strong tidal interactions. A nearby object is seen, but doesn't appear to disrupt the primary galaxy.
