The galaxy presents as a primarily smooth, elliptical object with a bright, concentrated central bulge. The overall form appears relatively undisturbed, exhibiting a lack of prominent spiral arms or major irregularities. The galaxy's light profile demonstrates a gradual decrease in intensity moving outward from the core, with no sharp truncations or distinct breaks observed. It has an intermediate roundness, not perfectly spherical but also not highly elongated. Faint color variations can be observed within the galaxy, with a slightly bluer hue in the outer regions, suggesting the presence of some star formation activity, though at a low level. There is a possible minor dust lane or region of obscuration present, but it is difficult to discern with certainty. The galaxy does not appear to be actively merging or interacting with any other large galaxies. Overall, it is a relatively quiescent galaxy.
