The galaxy presents a somewhat amorphous appearance. It exhibits a central, concentrated region of higher luminosity, surrounded by a more diffuse halo. The color profile shows a subtle variation, with the central region appearing slightly bluer than the outer halo, suggesting a possible difference in stellar population or star formation activity. The overall structure appears disturbed, potentially indicating an interaction with another galaxy or a recent merger event. There's no clear spiral arm structure evident, nor a distinct bar feature. Instead, the galaxy appears to be in a stage of transition, where the morphological classification is challenging. There are some possible tidal features present in the outer halo, suggesting there are disturbances that were caused by gravitational interactions. 
