The galaxy presents as a spiral type, characterized by a distinct, though somewhat ill-defined, central bulge. The spiral arms are prominent, extending outward from the central region in a relatively open, loose winding pattern. Two arms are the most apparent. There are hints of additional arms. The central bulge appears to have a moderate size relative to the overall structure.

A bar structure appears to be present, although the presence of a bar is not a certainty. The image suggests ongoing star formation, as indicated by the relatively high apparent brightness of the spiral arms. There are signs of potential tidal disturbances, with some asymmetry evident in the outer regions of the spiral arms, suggestive of a possible ongoing or recent interaction. The color profile of the spiral arms exhibits a blueish hue.
