The galaxy presents as a spiral type, exhibiting distinct, though somewhat ill-defined, spiral arm structures. Two primary arms are discernible, winding loosely from a central bulge. The bulge itself appears moderate in size and exhibits a yellowish hue, potentially indicative of an older stellar population. The spiral arms display a bluer color, suggesting ongoing star formation activity. There's also what appears to be a very small disturbance in the arm extending upwards in the image. No strong bar feature is readily apparent, although a subtle elongation may be present. Overall, the galaxy appears relatively undisturbed, without clear signs of major recent merging events.
