The galaxy presents a generally smooth morphology, exhibiting a slightly elongated, cigar-shaped structure. The light is concentrated towards the center. The core displays a bright, concentrated intensity, suggesting the presence of a significant population of older stars, or potentially an active galactic nucleus, though further spectral analysis would be required to confirm this.

The overall color appears bluish-white at the center, with a subtle shift toward redder hues at the lower edges. This color gradient hints at variations in stellar population or dust content across the galaxy. The relative smoothness of the galaxy suggests it is an elliptical galaxy. It appears relatively isolated, without signs of major interactions or mergers, though a possible minor disturbance cannot be completely ruled out given some slight asymmetry in its form.
