The galaxy presents a generally smooth, rounded morphology. There are no obvious spiral arms or bar structures visible. The light appears relatively concentrated towards the center, with a gradual decrease in intensity outward. The core region displays a yellowish hue, suggesting a population of older stars. Fainter, somewhat indistinct features extend outward from the central region, possibly indicating a weak disk or halo component. There is slight irregularity in the outer regions, perhaps due to minor gravitational interactions or internal activity. The galaxy's light profile appears relatively undisturbed overall, without major distortions or signs of an ongoing merger event, although some minor disturbances cannot be ruled out. The colors of the galaxy are predominantly in the redder wavelengths, with a faint blue-green present in some small outer regions of the galaxy, indicating there is some ongoing star formation, but the overall appearance suggests that star formation is largely suppressed.
