The galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is a prominent central bulge that is surrounded by a disk. The galaxy displays a smooth appearance, with no distinct spiral arm structure visible. The galaxy exhibits a moderate degree of roundness. There is some evidence of a minor disturbance or tidal tail extending from the galaxy, perhaps an indication of a recent interaction or merger. The colors are consistent with a mix of stellar populations, showing both older, redder stars and younger, bluer stars suggesting ongoing star formation.