This galaxy exhibits a moderately elliptical morphology, appearing somewhat elongated rather than perfectly spherical. The central region displays a concentrated luminosity, suggesting a significant stellar density or possibly an active galactic nucleus. The overall color profile tends towards the redder end of the spectrum, particularly in the core, which could indicate an older stellar population. Fainter, bluer regions extend from the central bulge, possibly indicating areas of recent or ongoing star formation. There is some evidence of asymmetrical features in the outer regions, which might imply tidal interactions or internal disturbances, though the disturbance appears minor. The galaxy seems to be relatively smooth in its overall structure.
