The galaxy presents as a moderately sized, well-defined object. It exhibits an elliptical morphology with a smooth appearance and no obvious spiral arm structure. The central region displays a high surface brightness, suggesting a concentrated stellar population or an active galactic nucleus. There appears to be a slight elongation, hinting at a possible flattened spheroidal shape. The color gradient transitions from a yellowish-white core to a bluer outer halo, suggesting a combination of older stellar populations concentrated in the center and younger, bluer stars in the periphery. There are subtle irregularities in the outer regions, potentially indicating minor disturbances or tidal interactions. Overall, the galaxy appears relatively undisturbed and not currently undergoing a major merger event.
