The galaxy presents as a moderately bright object with a generally smooth appearance, suggesting an elliptical morphology or a spiral galaxy viewed face-on without prominent spiral arms. There is a noticeable central bulge that is brighter and more concentrated than the surrounding galactic disk or halo. The bulge exhibits a yellowish-orange hue, which could indicate an older stellar population. Surrounding the central bulge, there's a more diffuse region of bluish light, suggesting more recent star formation, though it is subdued. The overall shape appears nearly circular, though there is a very slight elongation. There is no apparent evidence of strong tidal interactions or major mergers; however, some minor distortions might exist, warranting further investigation. The galaxy's light profile seems to fade gradually into the background, without abrupt edges. The color index implies the presence of both older and younger stars within the galaxy.
