The galaxy exhibits a morphology that is somewhat smooth, yet contains discernible features indicative of a disk structure. The overall shape is neither perfectly circular nor elongated, appearing somewhere in between these two extremes. There is a suggestion of some disturbance within the galactic structure, though whether this is a minor interaction with another galaxy or an internal phenomenon is not entirely clear from this imagery alone. The core of the galaxy presents a bright, concentrated region, with the light gradually diffusing outwards. Color gradients are apparent, with a yellowish hue dominating the central regions, possibly indicating an older stellar population. It shows signs of active star formation.
