The galaxy presents as an elliptical morphology, with a smooth, largely featureless structure. Its overall shape is close to circular. There is a concentrated central bulge with a bright, yellowish hue, suggesting a population of older stars. The galaxy appears relatively isolated, showing no strong signs of tidal interactions or mergers, though there may be a very slight asymmetry. The color gradients shift subtly outwards to redder hues. No distinct spiral arms or dust lanes are discernible. There is no evidence of active star formation.
