The galaxy presents as a relatively smooth, centrally concentrated object. A bright, yellowish core is observed, suggestive of an older stellar population. Moving outwards from the core, a faint, diffuse halo or disk-like structure is detected. The color of the outer regions appears slightly bluer than the core, hinting at possible ongoing star formation. There is no clear evidence of spiral arms, bars, or significant tidal disturbances. The overall morphology suggests a galaxy transitioning from a spiral structure to a more spheroidal shape or possibly an elliptical galaxy with ongoing star formation. There is no clear indication of any recent major merger events, although minor disturbances cannot be ruled out.
