The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, appearing as a flattened spheroid. The central region exhibits a high concentration of light, suggestive of a prominent galactic nucleus. The color profile indicates a likely older stellar population, with a yellowish-white hue dominating the core, gently transitioning to bluer tones in the outer regions, possibly indicating the presence of younger stars within a faint disk.

The galaxy lacks any clearly defined spiral arms. There is a subtle unevenness in the distribution of light in the outer regions, which could potentially point to minor gravitational interactions or past merger events, albeit without significant tidal tails or debris. The galaxy seems mostly undisturbed.
