The galaxy presents as a slightly elongated, disk-like structure, seen nearly edge-on. There is a central bulge with a moderate concentration of light, appearing yellow/orange in color, suggestive of an older stellar population. Fainter blue light extends along the plane of the disk. The galaxy disk is not perfectly symmetrical, with subtle irregular features. These irregularities could potentially be attributed to minor disturbances, possibly indicating ongoing or past interactions with another galaxy, however there are no other indications of recent merger events. No distinct spiral arm structures are immediately discernible at this resolution. The edges of the galaxy are not sharply defined, but rather fade into the background, suggesting a gradual decline in stellar density away from the central regions.
