The galaxy presents a primarily smooth, elliptical morphology, suggesting a relatively evolved system. The light distribution appears centrally concentrated, exhibiting a yellowish-red hue that is consistent with an older stellar population and low ongoing star formation. The galaxy has an axis ratio that indicates a slightly elongated shape. No distinct spiral arm structures or prominent dust lanes are discernible. The system shows no strong signs of major mergers, though a possibility of minor disturbances cannot be ruled out given the slight irregularity in its overall shape. Overall, the galaxy appears as a quiescent, relatively massive early-type galaxy.
