The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity towards its outer regions. The galaxy has a slightly elongated shape, deviating minimally from a perfectly circular morphology. Its color indices suggest an older stellar population, appearing more luminous in redder bands than bluer bands. There is a notable absence of any distinct spiral arm structures or prominent dust lanes. The galaxy does not appear to be undergoing any major mergers, although there is possibly a minor disturbance in its symmetry, suggesting potential interactions with smaller satellite galaxies. The overall structure implies a morphologically evolved system, with a high likelihood of hosting a supermassive black hole at its center. The estimated size is approximately 3 kpc across. Based on the colors, the star formation rate is estimated to be very low.
