The galaxy presents a generally smooth morphology, with a discernible lack of prominent spiral arms or distinct dust lanes. The overall shape is elongated, with a high axial ratio suggestive of an elliptical or lenticular galaxy viewed from an oblique angle. The central bulge is pronounced and appears brighter, exhibiting a reddish hue that potentially indicates an older stellar population. The outer regions of the galaxy gradually fade in intensity, displaying a slightly bluer tint, which may correspond to younger stars. Faint hints of possible disturbances or minor tidal features can be observed, potentially signifying past interactions or mergers. A single, compact object with a reddish color lies offset to the left of the main galaxy, suggestive of a satellite galaxy or background object. There appears to be no signs of major disturbances or ongoing mergers.
