This galaxy presents as a spiral type, exhibiting a prominent disk structure. The arms are well-defined, emanating from a central bulge. The color gradient suggests a population of younger, bluer stars within the spiral arms, indicative of ongoing star formation. There are also signs of older stars in the central bulge, with a redder color that shows a more progressed stellar population. The degree of winding appears tight, with a multitude of arm structures. There are no obvious signs of a strong bar feature bisecting the central region. There seems to be little to no evidence of a recent or ongoing major merger. Overall, the galaxy appears to be relatively undisturbed, showcasing its spiral morphology.