This galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. Moving outward from the core, the galaxy displays a subtle color gradient, shifting towards a slightly bluer hue. This hints at the presence of some ongoing star formation within the galaxy's outer regions, though not at a significantly high rate. There is no prominent disk structure or spiral arm features readily apparent. No major disturbances or signs of a recent merger are obviously visible. The light distribution appears relatively uniform and undisturbed.
