The galaxy presents a smooth, elliptical morphology. Its light distribution is centrally concentrated, diminishing outwards in a diffuse manner. The galaxy exhibits a pronounced bulge component dominating its overall structure. The ellipticity is moderate, deviating slightly from a perfectly circular form. Color gradients suggest that the central regions are relatively redder compared to the outer parts of the galaxy. There's an absence of readily discernible spiral arms or prominent dust lanes, further supporting its classification as an elliptical galaxy. Faint features surrounding the core may be indicative of a stellar halo or tidal debris, although at this resolution, detailed analysis of these features is limited. There may be minor disturbances, but overall the galaxy appears mostly undisturbed.
