The galaxy presents as a generally smooth, elliptical morphology with a highly concentrated central bulge. A faint, diffuse halo surrounds the brighter core, gradually fading into the background. The galaxy exhibits a noticeable color gradient, with the central region appearing redder, transitioning to a slightly bluer hue in the outer regions of the halo. This suggests a potential difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars present in the halo, indicating ongoing, though potentially low, star formation. No strong tidal features or distortions are apparent, implying it is relatively undisturbed, or that past disturbances are now fully incorporated into the galaxy's overall structure. The galaxy appears largely isolated, showing no obvious signs of interaction with other galaxies in its immediate vicinity.
