The galaxy appears as a relatively small, slightly elongated object. It exhibits a bright, concentrated central region which graduates to a more diffuse outer halo. The color gradient suggests a mixture of stellar populations, with the central region displaying a bluer hue, possibly indicating younger, hotter stars. The outer regions appear redder, suggesting an older stellar population or dust extinction. There is a subtle hint of irregularity or possible tidal features extending from one edge of the galaxy, which could be indicative of a past or ongoing minor merger event. The overall morphology leans towards a disk-like structure, although it appears somewhat perturbed. 
