The galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is a bright central bulge, somewhat spheroidal and exhibiting a yellowish or reddish hue, suggestive of an older stellar population. Extending from this central region is a faint, elongated disk. The disk structure displays hints of spiral arms, though their definition is somewhat indistinct. A portion of the disk exhibits a bluish coloration, possibly indicative of ongoing star formation within those regions. The overall structure suggests a system undergoing some form of minor interaction or disturbance.
