The galaxy presents as a lenticular structure, exhibiting a smooth, diffuse appearance with a subtle central bulge. The morphology suggests an evolved system, with a high fraction of older stellar populations. The overall shape is elliptical, tending toward an intermediate state, with a slight elongation. There are no obvious signs of active galactic nuclei, significant dust lanes, or prominent spiral arms. The color gradient across the galaxy is minimal, indicating a relatively homogeneous stellar population. No major mergers appear to be occurring, though there is some slight disturbance to the structure of the object. The galaxy is a relatively isolated object.

