The galaxy presents as a relatively compact object, appearing largely smooth and unstructured at this resolution. It exhibits a somewhat flattened spheroidal shape, with an aspect ratio suggesting it is not perfectly face-on. The light distribution is concentrated towards the center, indicating the presence of a bulge. Color gradients are subtle; a slightly bluer hue is noticeable in the central region, possibly suggesting ongoing or recent star formation activity. Overall, the galaxy seems to be relatively isolated, without any clear signs of tidal interactions or major disturbances in its morphology. It does not exhibit prominent spiral arms or a well-defined disk structure.
