The galaxy presents a generally smooth and rounded appearance. Its overall color profile appears to lean towards redder wavelengths, with a concentrated orange-ish hue in the core, suggesting an older stellar population dominating its composition. The galaxy appears to be relatively undisturbed. There is little to no evidence of spiral arm structure. The morphology appears elliptical or potentially lenticular. The galaxy seems well-defined, with a clear boundary between its luminous regions and the surrounding background. The galaxy does not show any signs of ongoing mergers or major interactions with other galaxies.
