The observed galaxy presents as a moderately sized, lenticular or elliptical system, elongated in shape. The galaxy exhibits a smooth, diffuse light distribution without any discernible spiral arm structure. The central region appears brighter and more concentrated, suggesting a central bulge. There is an apparent color gradient, with the central region displaying a yellower hue, which could be indicative of an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of younger, hotter stars, although this is not definitively evident given the limitations of the image resolution. The galaxy shows a relatively undisturbed morphology, without obvious signs of recent major mergers or tidal interactions. The edges of the galaxy fade gently into the background sky, showing no strong or hard edge. The galaxy appears to be relatively isolated.
