The galaxy presents a generally smooth, elliptical morphology. There is evidence of a disk-like structure. The galaxy exhibits a centrally concentrated luminosity profile, indicative of a significant bulge component, which is distinctly yellow, suggesting an older stellar population. There is bluer light emanating from other areas of the galaxy, indicating some active star formation. Overall, the light is dominated by the central yellow core. A minor disturbance could be occurring. The estimated size is consistent with that of an average spiral galaxy, with a notable central mass. 
