This galaxy appears to be a spiral, observed at an inclined angle. It presents a somewhat elongated, cigar-like shape. The central bulge is relatively prominent and exhibits a yellowish hue, suggesting an older stellar population with less ongoing star formation.

Fainter, bluer regions extending from the central bulge are also seen, indicating the presence of younger, hotter stars and potentially some ongoing star formation within the spiral arms. There is also a minor indication of a small amount of tidal disturbance, or at least a slightly asymmetric morphology, which suggests the possibility of a past interaction or merger event. Overall, the galaxy appears as a relatively quiescent spiral, with a moderate level of star formation.
