This galaxy presents a flattened, disk-like morphology. The central region exhibits a bright, concentrated core, possibly indicative of a bulge component. Surrounding this core is a fainter, extended disk. The color profile reveals a central blue-white area encircled by a pinkish hue that could be indicative of H-alpha emissions from star formation. The outer regions of the galaxy are poorly defined and more difficult to discern, seemingly diffuse. There appears to be a slight tidal disturbance within the galaxy, with a suggestion of a slight disruption, or perhaps an interaction event. No strong spiral arm structure is readily apparent. There are no evident signs of a complete merging event however there could be a sign of minor disturbances.