The galaxy presents as a moderately inclined, disk-shaped structure. Its overall color suggests a relatively mature stellar population, with a central bulge appearing brighter and slightly bluer than the outer regions of the disk. The morphological features indicate possible past or ongoing interactions, the disk shape being disturbed. There appear to be regions of star formation occurring. The galaxy also appears relatively smooth, lacking defined spiral arm structures, implying it could be an early-type spiral or potentially a lenticular galaxy. The light is centrally concentrated, suggesting an older and evolved system, with an effective radius of a few kiloparsecs.
