The galaxy presents as a spiral galaxy, with a clearly defined disk structure. Spiral arms are present, exhibiting a moderately wound morphology, that is mostly difficult to discern. The central bulge is relatively small and non-dominant. The galaxy has a general smooth appearance, suggesting a mixed stellar population. There is some hint of ongoing star formation within the spiral arms, indicated by bluer regions but it is not extreme. There is no strong evidence of a bar structure. The galaxy shows no significant signs of major tidal disturbances or a major ongoing merger. The galaxy appears to be relatively isolated, not displaying obvious interactions with nearby galaxies in this field of view.
