The galaxy presents as a moderately compact, somewhat luminous object with an apparent smooth morphology. The central region exhibits a brighter concentration of light, suggestive of a core or bulge component. The overall shape appears close to circular, though a slight elongation might be present. The galaxy displays a predominantly blue-white hue, potentially indicating the presence of a population of younger stars. There may be hints of a very faint disk structure or some diffuse, less structured regions surrounding the central bulge, although these features are not very pronounced. There is no obvious evidence of strong spiral arms or significant disturbances indicative of recent merger activity. The object is generally isolated, lacking any nearby companions that might suggest tidal interactions.
