The galaxy presents as a relatively compact and flattened disk structure. It exhibits a central bulge that is not particularly prominent. The disk is oriented at an angle, presenting an elongated shape. The color profile shows a bluer hue centrally, potentially indicative of ongoing star formation, with a gradual shift towards redder tones towards the outer edges. The disk appears somewhat featureless, lacking prominent spiral arm structures. The overall light distribution appears relatively smooth, possibly reflecting a more evolved stellar population in the outer regions.
