The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a dominant central bulge. There is a lack of any spiral arm structure or significant disk component apparent in this image. The overall shape appears generally rounded. A faint halo may surround the central region.

Based on its color profile, the galaxy exhibits a bluer hue. This suggests a population of younger stars. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances. There might be minor disturbances, however.
