The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge region exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by evolved stars. The outer regions of the galaxy appear fainter and subtly bluer, which may indicate some ongoing, albeit low, star formation activity within a more distributed disk. The galaxy appears elongated, with an approximate aspect ratio of 3:5, potentially indicating an elliptical morphology viewed at an oblique angle, or a lenticular morphology viewed at an oblique angle. There are no prominent spiral arms or dust lanes visible. There is no evidence of any major ongoing mergers or tidal disturbances. The overall morphology is relatively undisturbed, suggesting that it is an isolated galaxy that may have been created through a past major merger.
