The galaxy presents a primarily smooth, elliptical morphology. A concentrated central bulge dominates the luminosity profile, with light appearing to diminish gradually towards the outer regions. The overall shape is roughly round but slightly elongated along one axis. The color profile suggests an older stellar population, evidenced by the reddish-yellow hue. There is no visible evidence of strong spiral arm structures or significant dust lanes. Subtle irregularities in the outer regions hint at possible tidal interactions or minor disturbances, though no major merging events are immediately apparent.
