The galaxy presents as a somewhat elongated structure. Its color is primarily a yellowish hue. There is a hint of bluer light towards what appears to be the edges of the galaxy, suggesting some level of ongoing star formation in these regions. The central region appears smoother and redder, potentially indicative of an older stellar population. No obvious spiral arm structure is discernible, nor are any major distortions present. The overall form suggests a possible transition between an elliptical and a disk galaxy, or perhaps a lenticular classification. There may be some minor disturbances in the outer regions.
