The galaxy presents as a spiral, exhibiting well-defined spiral arm structures. These arms appear open and extend outwards from a central bulge. The bulge itself presents with a moderate size relative to the overall galaxy disk. There is a suggestion of a bar-like structure within the central region of the bulge, but it is not a highly prominent feature. The color distribution indicates a gradient, with the bulge showing a redder hue, potentially indicating a higher concentration of older stellar populations. The spiral arms show a mix of colors, with bluer patches suggestive of ongoing star formation. The galaxy shows no strong signs of tidal disruption or major merger activity; however, there are possible minor disturbances to the disk's symmetry. The disk is viewed at an angle closer to face-on.
