This galaxy presents as a flattened, disk-like structure oriented nearly edge-on to our line of sight. The central bulge appears bright and concentrated, exhibiting a smooth, spheroidal morphology. There is some distortion in the galaxy's shape, possibly due to minor gravitational interactions with other celestial bodies, although the main body of the galaxy appears relatively undisturbed. The stellar population appears evolved, with a dominant redder color indicative of older stars and a low rate of current star formation. The galaxy is relatively compact, but moderately massive. Overall, the galaxy seems to be an elliptical galaxy, with a quiescent nature and low specific star formation rate.
