The galaxy presents as a centrally concentrated, elliptical structure. It exhibits a smooth, diffuse morphology with minimal discernible features such as spiral arms or prominent dust lanes. The core region appears bright, indicating a potentially high concentration of stars or the presence of an active galactic nucleus. The overall color profile suggests a population of older stars, shifting towards redder wavelengths. However, some blue emission is seen, which could indicate ongoing star formation. There's evidence of possible tidal disturbances and potentially a minor merger event is in process. The estimated size is approximately 7.8 kiloparsecs across. The mass is estimated to be around 10^10.9 solar masses, with a star formation rate on the order of 10^0.5 solar masses per year.
