The galaxy presents as a spiral system, viewed at an angle between face-on and edge-on. A central bulge, exhibiting a yellowish hue, dominates the core region. Fainter spiral arms extend outwards. These arms display a bluer color, suggestive of ongoing star formation. A slight asymmetry can be observed in the outer regions. One side of the galaxy seems more extended, or perhaps slightly disrupted, with hints of redder regions, potentially indicating areas of dust obscuration or older stellar populations. Overall, it appears to be a moderately inclined spiral galaxy with evident star forming regions and a hint of possible interaction or recent perturbation.
