The galaxy presents as a central, bright bulge surrounded by a fainter, disk-like structure. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. The disk appears to be weakly defined with hints of spiral arms. The arms are not well-resolved, appearing somewhat flocculent. Some blue tinges are present in the disk region, possibly indicating areas of more recent star formation. The overall impression is that of a relatively quiescent galaxy, with moderate star formation activity. There is some evidence of disturbance, but the galaxy appears to be fairly stable. The galaxy appears to be relatively smooth in its structure and has round features. 
