The galaxy appears to be of elliptical morphology. It exhibits a predominantly smooth structure with minimal discernible features such as spiral arms or a distinct disk component. The central region displays a concentrated luminosity profile, suggesting a significant stellar population and/or an active galactic nucleus. The shape of the galaxy is roughly circular, with only minor deviations from perfect roundness. There is no visible evidence of ongoing or recent major mergers or tidal disturbances affecting the galaxy's overall structure. Faint wisps or extensions might be present in the outskirts but are largely obscured by background noise. The color profile is relatively uniform across the galaxy's body, indicating a consistent stellar population age, or that dust is not heavily obscuring any specific region. Overall, this galaxy presents as a relatively undisturbed, evolved system.
