The galaxy appears to be an elliptical galaxy, characterized by its smooth, generally featureless morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the nucleus, gradually decreasing outwards. The overall shape is more or less rounded, with a slight elongation. The color index suggests an older stellar population, with the galaxy appearing redder due to the presence of evolved stars and lower star formation rates. No spiral arms or significant dust lanes are discernible, consistent with the classification of an elliptical galaxy. There is no obvious evidence of any ongoing merging activity or tidal disturbances.
