The galaxy presents as a relatively compact, disk-shaped structure with a noticeable central bulge. The core exhibits a yellowish hue, potentially indicating an older stellar population. The disk itself appears slightly asymmetric, with hints of bluer regions suggesting ongoing star formation. These bluer regions are not strongly defined, but distributed sparsely. The overall light distribution suggests a classification leaning towards a spiral galaxy, however there are no strong spiral arms. There is also some visual indication of a minor interaction or disturbance.
