This galaxy exhibits a somewhat elongated, cigar-shaped morphology. Its light profile appears relatively smooth, suggesting a predominantly bulge-dominated structure. There is a slight color gradient across the galaxy, with the central region appearing bluer, potentially indicating ongoing star formation. The outer regions appear redder in comparison, perhaps due to an older stellar population. Overall, there is no obvious presence of strong spiral arm structures or significant dust lanes. Evidence suggests that this is a relatively quiescent system, without substantial merging or major disturbances present in this image.