The galaxy appears as a slightly elongated, elliptical-like structure. Its central region exhibits a concentrated, bright luminosity. The color profile suggests an older stellar population, with a noticeable reddish hue. The overall form is relatively smooth, lacking any prominent spiral arms or significant dust lanes visible at this resolution. There is a subtle suggestion of faint extended outer regions, gradually fading into the background. There are no indications of any recent major merger events or strong tidal disturbances. The galaxy appears relatively undisturbed.
