The galaxy presents as a relatively smooth, elliptical structure with a slightly elongated shape. A distinct central bulge exhibits a concentrated, yellowish-orange hue, indicating a population of older stars. Surrounding the bulge is a broader, less concentrated disk or halo, displaying a bluer color, suggestive of ongoing or recent star formation. There is a subtle hint of possible disk-like features, but these are not well-defined, and the overall morphology is dominated by the smooth, spheroidal component. No obvious signs of tidal disturbances, major mergers, or spiral arm structures are apparent. The galaxy appears to be relatively isolated and undisturbed.
