The galaxy presents a somewhat elongated morphology, appearing nearly edge-on from our vantage point. There is evidence of both a bulge and a disk component. The bulge appears bright and relatively smooth, with a concentrated luminosity profile. The disk is less distinct and seems to exhibit some level of disturbance or asymmetry. Faint tidal features are visible, suggesting a possible recent or ongoing interaction with another galaxy. Star formation appears to be ongoing, especially within the disk component.
