The galaxy presents as a centrally concentrated, smooth object. The light profile appears elliptical, with the isophotes showing a gradual decrease in intensity from the core outwards. The color gradient suggests an aging stellar population, with a yellowish-orange hue dominating the central bulge region. Fainter, bluer light extends subtly into the outer regions, possibly indicating some low-level recent star formation, though the bulk of the stellar population appears older. There's a subtle asymmetry in the outer disk, possibly indicating a minor tidal interaction or internal disturbance, however, overall, there are no prominent features such as spiral arms or a bar. It appears relatively undisturbed.
