The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration indicated by the bright core region. The overall color appears relatively red, suggesting a stellar population dominated by older, less massive stars, which is consistent with its classification. The isophotes are generally well-behaved, displaying a degree of flattening. There is little evidence of distinct spiral arm structures or significant dust lanes. The galaxy exhibits only minor disturbances, with no signs of active merging or major tidal features. Star formation appears to be relatively low. The galaxy is moderately luminous.
