The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a roughly elliptical morphology, appearing quite rounded. There's a gradual decrease in light intensity from the core outwards, with no discernible spiral arm structures or prominent dust lanes visible. The color profile suggests a relatively evolved stellar population, trending towards redder hues in the central regions, indicative of older, cooler stars. The outer regions present slightly bluer tones, possibly from younger stars. There appears to be a minor disturbance, or faint asymmetry. Overall, the galaxy appears as a relatively undisturbed, evolved system, potentially an elliptical or lenticular galaxy.
