The galaxy presents as a moderately sized, lenticular or possibly spiral galaxy, viewed at a significant angle relative to its face-on orientation. A bright, concentrated central bulge dominates the overall structure, exhibiting a smooth, symmetrical appearance. The disk surrounding the bulge appears relatively faint and thin, showing some evidence of spiral arm structure and is weakly defined. The galaxy's light appears to show an obvious blue shift. There is some minor evidence of asymmetry within the disk, but this could potentially be due to tidal interactions or dust lane irregularities. Overall, the galaxy appears relatively isolated and shows no obvious signs of a major merger event.
