The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It presents a centrally concentrated luminosity profile, with brightness decreasing gradually from the core to the outer regions. The galaxy possesses a slightly elongated shape; it is neither perfectly spherical nor highly flattened. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy's color suggests a stellar population dominated by older, redder stars, typical of elliptical galaxies. There may be some indications of on-going or recent star formation, which could explain the slight blueness in color. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances based on its overall structure.
