The galaxy presents as a well-defined, flattened disk galaxy, observed nearly edge-on from our line of sight. A prominent central bulge appears bright and concentrated, exhibiting a yellow-orange hue indicative of an older stellar population. The disk is visible extending outwards from the bulge. The disk appears to be slightly warped. The galaxy displays an overall smooth texture with little signs of dust lanes or prominent spiral arm structures. The galaxy is relatively isolated, showing no strong signs of tidal disturbances or ongoing mergers, but perhaps some minor interactions. The color gradient suggests a decrease in the average stellar age from the center to the outer regions of the disk.
