The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. It displays a concentrated central bulge that is bright, with a yellow-orange hue, suggesting a population of older stars dominating the core. The galaxy fades gradually into a less luminous halo extending outwards from the central region. The overall shape is elongated with a relatively high axial ratio, indicating a somewhat flattened ellipsoid structure. There is no discernible evidence of prominent spiral arms or significant dust lanes. The galaxy appears to be relatively undisturbed, without any visible signs of tidal interactions or recent mergers. Its colour profile suggests a relatively low rate of ongoing star formation.
