The galaxy presents as a relatively smooth, elliptical-like structure, elongated along a discernible axis. A bright, concentrated central bulge is visible, appearing yellowish in color. Fainter, bluish-white light extends outwards from this central region, suggesting the presence of a stellar disk, although it appears fairly compact. The overall color gradients suggest a relatively evolved stellar population, although some ongoing star formation cannot be ruled out based on the bluer regions within the disk. There is a subtle asymmetry present in the outer regions of the galaxy, perhaps indicative of a minor tidal interaction or past merger event, however, it is difficult to confirm that.
