The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. There is a dominant central bulge, which appears approximately spherical and emits a bright, white-yellow light. The outer regions of the galaxy exhibit a diffuse, disk-like structure, subtly bluer in color compared to the central bulge. This suggests ongoing, though perhaps subdued, star formation in the disk component. There are no clear signs of strong spiral arm structure, or any signs of current major merger activity, though there appears to be slight distortion suggesting a possible minor interaction or past disturbance. The galaxy's overall appearance aligns with that of an early-type spiral or a lenticular galaxy.
