The observed galaxy presents as a roughly elliptical form, elongated along a horizontal axis. The central region exhibits high surface brightness, appearing nearly uniform in color. A diffuse halo surrounds the central body, characterized by a bluer hue. There is evidence of a disk-like structure. Based on the lack of distinct spiral arm structure, and a high level of smoothness, the galaxy is most likely an elliptical galaxy. There is minimal evidence of any significant tidal distortions or mergers, though there is potential disturbance in its structure.
