This galaxy presents as a slightly inclined, well-defined spiral structure. Two prominent spiral arms are observed, extending from a central bulge. The arms display medium winding. The central bulge appears moderate in size and exhibits a yellowish hue, suggesting an older stellar population. The spiral arms show regions of bluer color, indicative of ongoing star formation. There does not appear to be a strong central bar, although there is a hint of a weak bar. The disk appears relatively smooth, but exhibits some irregularities, with one side slightly more extended than the other. Overall, there is no indication of a major merger or significant tidal disruption.