The galaxy presents as a somewhat smooth, disk-like structure. It exhibits a central bulge that appears yellowish-orange in color, suggesting an older stellar population. Surrounding the bulge is a fainter disk with hints of blue-green hues, which may indicate more recent star formation within this region. There is no apparent bar structure or strong spiral arm presence, instead there are hints of disturbed features. The edges of the galaxy fade gradually into the background, making it difficult to determine its exact boundaries. Overall, the galaxy appears to be relatively undisturbed, without obvious signs of a major ongoing merger, although there may be evidence of recent or ongoing minor disturbances.
