The galaxy presents as an elliptical or lenticular type, with a predominantly smooth and rounded morphology. There is a suggestion of a central bulge with a high concentration of light, appearing yellowish-white. Diffuse reddish areas are subtly distributed throughout the galaxy, particularly in the outer regions. These may indicate areas of dust obscuration, or possibly regions of older stellar populations with lower rates of star formation, based on the relative brightness in different wavelengths of light. There is little to no evidence of spiral arm structure or strong tidal disturbances, suggesting a relatively quiescent or undisturbed history. Overall, the galaxy exhibits a relatively homogenous distribution of light with a somewhat elliptical shape.
