The galaxy exhibits a generally smooth morphology, indicating an elliptical or lenticular classification. The central region presents a concentrated, bright core. Proceeding outward, the luminosity gradually decreases, forming a somewhat elliptical shape. A faint disk appears to be present when observing at its maximum diameter. A very slight disturbance can be seen at the outer edges of this disk, indicating the possibility of a minor interaction with another galaxy at some point in its past. The color gradient transitions from yellowish-white at its core to a more greenish hue at its outer edges, suggestive of aging stellar populations in its central bulge, and a small amount of star formation occurring in the outer arms of the faint disk.
