The galaxy presents an overall smooth, elongated morphology. Its light profile appears relatively uniform across the visible extent, showing little to no evidence of spiral arms or prominent structures. The central region exhibits a slight concentration of light, though not sharply defined, suggesting a subtle bulge. The color is generally blueish-white, hinting at a population of younger stars and possibly ongoing, though subdued, star formation. There are no obvious signs of active galactic nuclei activity or significant dust lanes. It appears to be a lenticular or possibly a small elliptical galaxy. The disk is noticeably elongated. There may be a very slight indication of disturbance on the edges of the galaxy, but it is very faint.
