The galaxy presents as a single, somewhat smooth, and centrally concentrated light source. It exhibits a generally elliptical morphology, appearing largely round with a very slight suggestion of elongation. There is a strong central bulge that dominates the overall light profile. The galaxy shows a primarily yellow-orange hue, transitioning to slightly redder tones in the central region. Fainter, diffuse blue-green extensions are subtly apparent in the outer regions, potentially indicating areas of more recent, but overall low, star formation. There is no obvious indication of spiral arms or a well-defined disk structure. No significant tidal disturbances or close companion galaxies are readily visible, although there is a very slight suggestion of a minor disturbance in the outer reaches of the galaxy.
