The galaxy presents as a distinct, elongated structure. It exhibits a pronounced central bulge with a yellowish-orange hue, suggesting an older stellar population concentrated in the core. Extending outwards from this bulge are fainter, bluish-white extensions, possibly indicative of a disk component with ongoing star formation. The elongation suggests the galaxy is either a highly inclined spiral or a prolate elliptical. There is no clear indication of prominent spiral arms. The overall morphology appears relatively undisturbed, without strong signs of a major merger event, though there could be a faint tidal stream or minor disturbance contributing to the irregularity of the disk.
