The galaxy exhibits a fairly smooth morphology, suggesting it may be an elliptical or lenticular type. There's a concentrated, bright central bulge, surrounded by a more diffuse, extended halo. The galaxy's light profile appears highly concentrated, with a lack of distinct spiral arm structures. The overall color is slightly red, which implies an older stellar population and lower rate of star formation. There seems to be a slight distortion that could be due to a gravitational interaction with another galaxy, although there are no clear signs of a recent major merger.
