The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that diminishes gradually in luminosity towards the outer edges. The shape is not perfectly circular, showing a slight elongation. There is a subtle color gradient, with the central bulge appearing more yellow-orange compared to the slightly bluer hues of the outer regions. There is little indication of prominent spiral arm structures or significant dust lanes, lending further support to the galaxy's classification as an elliptical type. There appears to be no strong evidence of ongoing major merging events or tidal disturbances, although the possibility of minor interaction cannot be ruled out.
