The galaxy presents as a moderately bright, relatively compact object with a smooth, elliptical morphology. It appears largely featureless, lacking distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, indicated by the yellowish-red hue. The central region is brighter and more concentrated, likely representing a substantial bulge component. There might be a subtle, very faint extended halo surrounding the central region. No evidence of active galactic nuclei or recent major mergers is immediately apparent in the visual data.