The galaxy presents as a spiral with a prominent central bulge. The bulge exhibits a bright, relatively uniform distribution of light, with a slightly bluish hue suggesting a population of younger stars. The spiral arms are well-defined, winding relatively tightly around the bulge. They are noticeably bluer than the bulge, indicative of ongoing star formation. The galaxy appears to have at least two dominant spiral arms, possibly more, although the exact number is somewhat obscured by the image resolution. There is a suggestion of a bar structure present across the central region, though it is not particularly strong. No significant signs of major mergers or tidal disturbances are immediately apparent, though there may be minor asymmetries in the outer regions of the disk.
