The galaxy presents as a somewhat elliptical, though noticeably oblong, structure with a smooth, diffuse light distribution. A centrally concentrated bulge region exhibits a yellowish-white hue, suggesting a population of older stars. The surrounding disk appears fainter, with subtle hints of bluer tones in some regions, potentially indicating younger star formation. There is a slight visual distortion in the structure that could indicate a weak tidal interaction or an internal asymmetry. The disk fades gradually into the background, with no clear evidence of strong spiral arms or distinct features.
