The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a bright, concentrated central bulge which comprises a significant portion of its overall luminosity. There is a decrease in luminosity emanating outward from this central region, which is fairly symmetric. The galaxy has a smooth appearance with minimal visual evidence of spiral arms or distinct substructures. Its overall shape is approximately circular, with no obvious elongation or tidal features suggesting a recent major merger event. The observed color profile indicates a population of older stars; no regions of intense blue light are visible, and the light is slightly redder. The data is of low resolution and the galaxy is relatively small, which is likely why there is an inability to resolve further detailed features within the galaxy's structure. It appears to have a companion galaxy close to the right of the galaxy.
