The galaxy appears as a highly inclined, disk-shaped system. It is seen nearly edge-on, obscuring much of the internal structure. The central region exhibits a pronounced bulge, appearing brighter and more concentrated than the outer disk. This central bulge exhibits a yellowish hue. The disk itself presents a bluer color gradient extending outwards. There is no strong evidence of ongoing major merging activity or significant tidal disturbances in this image. Faint dust lanes are suspected within the disk, although the high inclination and resolution limitations make definitive identification difficult. Star formation is likely present but appears to be fairly subdued.
