The galaxy presents as a moderately luminous, elliptical or lenticular system. Its overall color is yellowish, indicating a population of older stars with lower rates of current star formation. The galaxy exhibits a smooth, concentrated light profile, with no apparent spiral arm structures or significant dust lanes. The isophotes appear generally regular, suggesting a relaxed morphology, although there might be a very slight asymmetry or minor disturbance visible in the outer regions. The galaxy does not appear to be undergoing any major merger activity and is relatively isolated in the field. Its compactness suggests it is a moderately massive system.
