The galaxy presents as a disk galaxy, although it's inclination prevents precise classification. The central bulge appears prominent and exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the bulge, the disk becomes more bluish and less distinct. There is a relatively smooth texture throughout the galaxy. The disk is elongated and appears to have only minor disruptions to its structure. There is no evidence of significant ongoing mergers or major tidal disturbances. Overall, the galaxy appears to be relatively undisturbed. 
