The galaxy presents as a centrally concentrated, luminous object with a generally smooth morphology. Its shape is largely elliptical, deviating slightly from a perfect circle. The light distribution indicates a significant bulge component, with a high concentration of older stars likely dominating the central region, emitting primarily in the redder wavelengths.

Fainter, diffuse light surrounds the central bulge, suggesting the presence of a disk component or an extended halo of stars. Hints of bluer colors in the outer regions indicate some ongoing star formation, although it appears relatively subdued. There is also an indication of a minor tidal disturbance in the outer regions, possibly due to a past or ongoing interaction with a smaller galaxy, but the main body appears largely undisturbed. Overall, this galaxy appears to be an intermediate-mass system, transitioning from a more actively star-forming spiral towards a passively evolving elliptical galaxy.
