The galaxy presents as a largely smooth, elliptical object. It exhibits a bright, concentrated central bulge, indicative of a high stellar density. The isophotes appear generally regular, with a slightly elongated shape, suggesting a classification between round and cigar-shaped. There is some visual evidence of a faint disk component, subtly embedded within the overall smooth appearance. A marginal disturbance can be observed but no major mergers seem to be occurring. Color gradients within the galaxy suggest a radial distribution of stellar populations, with bluer colors present in the outer regions and a progression towards redder colors in the nucleus. The overall morphology is generally undisturbed, showing no indication of strong tidal interactions or major recent merger events.
