The galaxy presents a roughly elliptical morphology, though not perfectly circular. It appears to have a prominent central bulge, exhibiting a concentrated, yellowish hue. Extending outward from the bulge, fainter, bluer regions are visible, potentially indicating the presence of spiral arms or a disk component. Some irregularities are observed in the outer regions of the disk, hinting at possible tidal interactions or recent minor mergers. There is no evidence of a strong tidal tail, but a slightly disturbed morphology suggests ongoing or recent interactions. The overall color gradient suggests a mix of older stellar populations concentrated in the bulge and younger, star-forming regions in the disk.
