This galaxy presents an overall smooth appearance, though some subtle features are present. The central region exhibits a bright, concentrated core, likely the galactic nucleus. Surrounding the core is an extended, somewhat flattened disk or halo structure. Within the disk, there are hints of spiral arm structures, though they are not sharply defined; rather, they appear as broad, diffuse extensions emanating from the central region. The galaxy's color profile suggests ongoing star formation, with bluer hues observed in the outer regions, indicating the presence of younger, hotter stars. The galaxy has an intermediate shape between round and elongated. There is a suggestion of a minor gravitational disturbance possibly due to an interaction with a nearby object. The overall morphology appears to be that of a spiral galaxy undergoing some form of interaction or disturbance.
