The galaxy presents as a somewhat smooth, elliptical-like structure. It appears elongated in shape, being much longer than it is wide. The central region exhibits a bright, concentrated core, which gradually diffuses into the outer regions of the galaxy. The color profile indicates a generally older stellar population, with a yellowish hue dominating the central region, although the colors tend towards the blue end of the spectrum. There is no strong evidence of spiral arm structures or significant dust lanes. Faint, asymmetrical extensions or tidal features may be present, hinting at possible past interactions or mergers, but these are not pronounced.
