The galaxy exhibits a well-defined spiral structure. Two prominent spiral arms emanate from a central bulge, with the arms appearing grand design in nature. The arms display varying degrees of winding tightness, with some regions exhibiting a more tightly wound morphology while others appear more open. The central bulge appears moderate in size, contributing a significant portion to the overall luminosity of the galaxy. There is a suggestion of a bar feature crossing the central bulge, although the presence of dust lanes obscures a clear view of its strength. The galaxy's disk component displays a range of colors, with bluish hues suggesting the presence of younger stellar populations in the spiral arms and yellowish hues indicating older populations in the bulge and inner disk. There appears to be no significant sign of an ongoing major merger or tidal disruption, but some minor asymmetry in the spiral arms may hint at minor interactions or internal instabilities.
