The galaxy presents a morphology that appears primarily smooth, with a notable central concentration of luminosity. It exhibits a roughly elliptical shape, appearing somewhat elongated rather than perfectly circular. The overall color profile suggests a relatively uniform stellar population, potentially indicating an older, less actively star-forming system. There is a subtle indication of possible minor tidal disturbances in the outer regions of the galaxy, but overall, the structure appears relatively undisturbed. There does not seem to be a prominent spiral disk, and any internal features such as spiral arms or dust lanes, if present, are not readily discernible at this resolution. The apparent color suggests the presence of older stellar populations and reduced ongoing star formation.
