The galaxy presents as a flattened, elliptical morphology. Its light profile exhibits a smooth distribution, with a noticeable concentration towards the central region. The color gradient shifts from a generally bluer hue in the outer regions to a more yellow/red-shifted hue in the center. This may indicate a difference in stellar population, suggesting older stars reside in the galactic center.

The shape of the galaxy appears to be more oblong, lacking a completely spherical form. No distinct spiral arm structures or dust lanes are visible. There may be a slight asymmetry on one end, potentially indicative of a minor gravitational disturbance or interaction. However, the primary shape is consistent with a relatively relaxed, non-merging system.
