The galaxy presents as a relatively smooth, centrally concentrated object. The light profile suggests a lack of distinct spiral arms or a prominent disk structure. The central region exhibits a yellowish-white hue, indicative of an older stellar population. Moving outward from the center, the color gradually shifts to a redder tone. The galaxy appears to be elliptical or possibly a lenticular galaxy viewed face-on, with no significant signs of ongoing major mergers or tidal disturbances. A very minor asymmetric feature may be present in the outer regions, suggesting a possible past interaction or minor disturbance.
