The galaxy presents as a relatively smooth, elliptical morphology, with a concentrated central bulge. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central regions. The outer regions exhibit a slightly bluer tint, possibly indicating the presence of younger stars, though star formation appears to be suppressed overall. The galaxy lacks any prominent spiral arm structure or dust lanes, further supporting its classification as an elliptical type. There is no apparent strong tidal distortion or signs of ongoing major merger activity, but some minor asymmetries could indicate a past interaction. The light distribution is relatively uniform, fading gradually from the bright core towards the outer edges, with an estimated effective radius of a few kiloparsecs.
