The galaxy appears to be a spiral galaxy, viewed at an oblique angle. The central bulge is distinctly yellowish, implying an older stellar population. Faint spiral arms emanate from the bulge, exhibiting a slightly bluer tint. This suggests the presence of ongoing star formation in the arms, though the overall star formation rate seems relatively low. The galaxy's shape is generally intermediate between round and elongated. There is no obvious sign of any major ongoing merger or significant tidal disturbance. The galaxy's morphology seems largely undisturbed.
