The galaxy presents as a flattened, elongated structure, suggestive of a possible edge-on spiral or lenticular morphology. The central region exhibits a higher surface brightness, appearing nearly smooth with a yellow tint and a faint, diffuse bulge, possibly indicative of an older stellar population. Extending outwards from the core along the major axis are faint blue tinged arms. The relative smoothness and cigar shape also suggest a classification leaning towards an elliptical galaxy, viewed at an angle that does not reveal significant internal structure. There is no obvious evidence of a recent major merger, however there does appear to be some subtle disturbance or asymmetry in the outer regions. 
