The galaxy appears to be an elliptical galaxy, presenting a smooth, diffuse light profile without readily apparent spiral arm structures or dust lanes. The color is predominantly yellowish-orange in the central region, suggesting an older stellar population. The galaxy exhibits a high degree of radial symmetry, with the isophotes appearing mostly circular but perhaps slightly elongated. There is no indication of active star formation, with no blue or ultraviolet light emissions visible. There is no sign of tidal tails, bridges, or other morphological disturbances which leads to the interpretation that there is likely no current or recent major merger event occurring.
