The galaxy appears to be an elliptical galaxy, possessing a smooth, largely featureless morphology. The galaxy exhibits a concentrated central bulge that appears nearly spherical. There is a gradual falloff in luminosity from the core to the outer regions of the galaxy, with no distinct spiral arm structures or prominent dust lanes visible. It exhibits a color gradient, appearing more yellow-orange in the central regions, which may indicate a population of older stars. The outer regions exhibit a slightly bluer hue, potentially indicating a small population of younger stars. There is no obvious sign of a major ongoing merger or significant tidal disturbances, although there is a slight asymetry in the outer regions. The galaxy appears relatively isolated. Overall, it presents as a relatively mature, quiescent system.
