The galaxy presents as a slightly elongated structure, possibly an elliptical galaxy, or a spiral galaxy viewed at an angle. It exhibits a concentrated central bulge with a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer regions are observable extending from the central bulge, hinting at the presence of a disk with some star formation activity. A slight distortion or asymmetry may be present in the outer regions, possibly indicating past or ongoing gravitational interactions. The object displays a relatively smooth overall appearance with some subtle features in its disk, though is dominated by the bulge. The color profile is dominated by redder wavelengths.
