The galaxy presents a somewhat elliptical morphology, appearing largely smooth in structure. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in surface brightness towards the outer regions. There are hints of a faint disk structure.

The galaxy's color profile suggests a dominant population of older stars, as evidenced by its redder hue, although there are some areas that appear slightly bluer, possibly indicating pockets of recent or ongoing star formation. It is likely a relatively massive galaxy. There appear to be no major tidal distortions or signs of ongoing major mergers, though a possible minor disturbance or interaction cannot be ruled out based on the available imagery.
