The galaxy presents as a spiral type, exhibiting a distinct disk structure. Two prominent spiral arms are visible, displaying a moderately open winding. The arms appear somewhat flocculent, with intermittent regions of higher luminosity suggestive of active star formation. The central bulge appears relatively moderate in size, contributing a significant portion of the overall light. The bulge exhibits a yellowish-white hue, indicating an older stellar population. There is a subtle hint of a bar-like structure within the central region, but it does not appear to be overly pronounced. The disk shows a bluer color, consistent with the presence of younger, hotter stars within the spiral arms. There is no obvious evidence of a major merger event, although subtle disturbances or asymmetries within the spiral arm structure suggest the possibility of minor interactions. Overall, this galaxy presents as a fairly typical spiral galaxy with ongoing star formation and a relatively well-defined structure.
