The galaxy appears as a lenticular or early-type spiral galaxy. Its shape is elongated, showing a cigar-like form. The central bulge is a bright yellow, suggesting an older stellar population. Fainter, bluer light is observed in the outer regions, hinting at a low level of ongoing star formation within a disk structure. The overall structure is smooth with no visible signs of major disturbances or merging events. It appears to be a relatively isolated system.
