The galaxy presents a predominantly smooth morphology, with a concentrated central bulge exhibiting a bright, yellowish-white hue. A faint disk component appears to be present, oriented roughly edge-on. There is a slight hint of bluer color within the disk region, possibly indicating ongoing star formation. The galaxy is moderately large and is relatively circular in shape. There is evidence of some minor disturbances potentially indicative of a past or ongoing interaction or merger event. The mass of the galaxy is estimated to be quite substantial, with moderate star formation rates. Overall, the galaxy appears to be a relatively evolved system with characteristics of both an elliptical and a spiral galaxy.
