The galaxy presents as a single, relatively smooth object. The overall shape is elliptical or spheroidal, appearing more "in between" round and elliptical, lacking any discernible spiral arm structures. The central region exhibits a strong concentration of light, suggesting the presence of a substantial galactic bulge, possibly housing a supermassive black hole. The galaxy's color profile indicates a prominent red sequence, with a strong presence in the redder bands, suggesting an older stellar population with relatively lower levels of ongoing star formation. The galaxy appears to be relatively isolated with no obvious tidal features or interactions with neighboring galaxies, although there is a possible faint halo extending outwards. The size is moderate; it is neither extremely compact nor particularly large. The galaxy does not appear to be undergoing a major merger event or have strong internal disturbances.
