The galaxy presents as a spiral galaxy, viewed at an angle that is nearly face-on. Two distinct spiral arms are clearly visible and appear to have a medium winding. The arms emanate from a moderate-sized central bulge, which exhibits a yellowish hue, suggesting an older stellar population. This implies that the galaxy is actively forming stars in the spiral arms. The disk of the galaxy appears relatively undisturbed, with no significant signs of major mergers or tidal disruptions, though some minor disturbances cannot be ruled out at this resolution. There may be some slight evidence of a bar, extending across the center. The galaxy presents with a range of colors, suggestive of a stellar population of varying ages and compositions.
