The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. The core displays a bright, yellowish hue suggesting an older stellar population. Moving outwards, the color gradually transitions to a reddish tint, indicative of cooler stars and potentially some dust absorption. There appears to be a faint disk with some disturbance, indicating possible recent merger activity. The overall shape is predominantly round, but there is an indication of a slight elongation along one axis. The galaxy is moderately luminous and appears to be undergoing low rates of star formation.
