The galaxy presents as a single, relatively smooth object with a slight elongation. The central region appears brighter and exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually, showing a subtle color gradient towards a redder, less intense light. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears largely undisturbed, without obvious signs of ongoing major merger activity, although some subtle irregularity in the outer isophotes cannot be ruled out. The overall morphology is consistent with an elliptical galaxy or possibly a lenticular galaxy viewed at a shallow inclination.
