The galaxy presents as a relatively compact, elliptical-like structure with a concentrated central bulge. The light distribution appears smooth and largely featureless, lacking prominent spiral arms or distinct dust lanes. The galaxy is moderately bright, with a color profile that suggests a population of older stars, potentially indicative of a lower star formation rate. The overall shape is somewhat elongated but not exceptionally so, leaning towards a shape between round and cigar shaped. There are no obvious signs of ongoing major mergers or significant tidal disturbances.
