The galaxy presents as a somewhat elongated, elliptical-like object, exhibiting a smooth, concentrated light profile. The central region displays a bright, diffuse glow, suggestive of a high stellar density. The galaxy appears to be a mature system, lacking prominent spiral arms or distinct dust lanes. Color gradients suggest an older stellar population with redder hues dominating the central region, transitioning to slightly bluer tones in the outer regions, possibly indicating some ongoing, though subdued, star formation activity. There is no apparent evidence of strong tidal interactions or recent mergers, with a generally undisturbed morphology.
