The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses into a fainter, extended halo. The color profile indicates a redder hue, particularly in the central regions, suggesting an older stellar population with limited ongoing star formation. There is no obvious indication of spiral arm structure or dust lanes. The galaxy appears largely undisturbed, with no apparent signs of tidal interactions or recent mergers. It exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. The apparent size of the galaxy is relatively small, indicating a low intrinsic physical size.
