The galaxy exhibits a generally smooth morphology. The central region is characterized by a bright, concentrated bulge, possibly indicative of an older stellar population. Moving outward from the center, the light distribution becomes less concentrated. Faint disc-like features can be observed. There is also some evidence of minor disturbances in the outer regions of the galaxy, suggesting possible past interactions or mergers. The overall shape is between round and elongated, showing a somewhat elliptical appearance. The color distribution suggests ongoing star formation.
