The galaxy presents a complex morphology, exhibiting characteristics intermediate between elliptical and disk galaxies. Its overall shape is not perfectly spherical, showing a slight elongation. The central bulge is relatively prominent and appears to be composed of older stellar populations, evidenced by its yellowish hue. Surrounding the bulge, a fainter disk component is discernible, showing hints of bluer colors, suggestive of younger star formation regions. The disk appears somewhat disturbed or irregular, possibly indicating gravitational interaction with a companion or a past merger event. There may be signs of minor tidal features or disturbances in the outer regions of the galaxy, though these are faint and not definitive.
