The galaxy presents as an elliptical structure, seemingly devoid of prominent spiral arms or a significant disk component. The light distribution is centrally concentrated, exhibiting a smooth, relatively featureless morphology. There is a gradual decrease in luminosity moving outwards from the core, although the resolution limits a thorough investigation of its outer regions. The overall color appears to be dominated by redder wavelengths, suggestive of an older stellar population with a lower rate of ongoing star formation. There may be minor disturbances or tidal features present upon closer inspection, but none are immediately apparent. Based on the shape, it has high circular symmetry.
