The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. It is elliptical in shape, displaying a high degree of roundness. The central region exhibits a bright, yellowish-white core, indicative of an older stellar population. Moving outward from the core, a subtle color gradient towards bluish hues is observed. This suggests the presence of some ongoing, albeit modest, star formation in the outer regions. There is no discernible spiral arm structure or bar feature. The galaxy appears undisturbed, with no signs of major mergers or tidal disruptions. Faint extensions may exist, but these are difficult to distinguish clearly.
