The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-white hue, indicating a population of older stars. The galaxy appears somewhat rounded in shape. Faint extensions are present, subtly hinting at a possible disk structure, but it appears largely featureless. There's no evident indication of active star formation or significant dust lanes within the visible spectrum. There's no morphological evidence of recent or ongoing major mergers, but possibly some minor gravitational disturbance.
