The galaxy presents as a disk galaxy, likely viewed at a near edge-on orientation. A distinct bulge is visible, appearing slightly yellow and concentrated. Dust lanes appear to attenuate the light emanating from the disk, particularly near the central bulge. The disk itself exhibits a mottled texture, possibly indicative of ongoing star formation regions, with regions of bluer light interspersed with areas of slightly redder hue. The galaxy displays some evidence of disturbance or interaction, with an asymmetry visible in the outer regions of the disk, possibly influenced by minor gravitational interactions. Overall, the galaxy appears to be relatively massive, displaying a mix of old and young stellar populations and some recent or ongoing star formation activity. There are no obvious signs of a recent major merger.