The galaxy presents a generally smooth and rounded morphology, with a concentrated central region appearing nearly spheroidal. No obvious spiral arms, bars, or other distinct features are readily apparent in the image. The color profile indicates a yellow/white hue concentrated in the center, suggesting an older stellar population dominating the core. Fainter, slightly bluer extensions are observed around the central region but show no apparent structure. Evidence of tidal disturbances or ongoing mergers is not immediately visible; the galaxy appears relatively undisturbed. The absence of prominent dust lanes and the overall smooth appearance indicate that the galaxy is likely a massive system with low rates of current star formation.
