The galaxy presents as a fairly smooth, centrally concentrated light distribution. It appears largely elliptical in shape, exhibiting a high degree of rotational symmetry. There is a subtle color gradient, trending from a more yellow hue in the central region to slightly redder tones in the outer parts of the galaxy. No distinct spiral arms or prominent dust lanes are visible. A faint, elongated structure is observable at the bottom of the galaxy, potentially indicating a minor tidal disturbance or interaction with a smaller companion galaxy. The overall morphology suggests an evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed at a high inclination. Star formation activity appears low based on the dominant redder colors. The galaxy appears fairly isolated, with no other large galaxies in close proximity within the immediate field of view.
