The galaxy presents as a relatively face-on spiral, though with a notable lack of distinct spiral arm structure. It exhibits a bright, concentrated central bulge, characteristic of an older stellar population. The disk surrounding the bulge appears smooth and shows a subtle color gradient, transitioning from a more yellow/orange hue in the central regions to a slightly bluer tint in the outer edges. This suggests a difference in stellar populations, with younger, bluer stars residing preferentially in the outer disk. There is a hint of dust lane structure, especially apparent on the edges, causing some irregularities in the galaxy's profile. No significant signs of tidal disturbances or interactions are visible. Overall, the galaxy appears to be a relatively quiescent, evolved spiral galaxy.
