The galaxy presents as a flattened elliptical shape, appearing more like a disk when compared to perfect circles. It exhibits a smooth, featureless structure without any prominent spiral arms or distinct dust lanes visible in this observation.

The central region is notably brighter and concentrated, suggesting a high density of stars and potentially a supermassive black hole at its core. Moving outward from the core, the luminosity gradually decreases.

The overall color profile indicates that this galaxy is relatively red and yellow, implying a population of older stars. Blue regions are absent, suggesting minimal ongoing star formation.
