The galaxy presents a largely smooth morphology, lacking readily discernible spiral arms or a distinct bar structure. The light distribution appears concentrated towards the center, suggesting a prominent bulge component. Color gradients indicate a relatively red color in the core region, possibly indicative of an older stellar population. The outer regions show a slightly bluer color. There's some faint indication of possible tidal disturbances. Overall, the galaxy appears to be an elliptical galaxy or potentially a spiral galaxy observed at a high inclination, or an irregular galaxy undergoing some disturbance.
