The galaxy presents as an edge-on spiral with a prominent central bulge exhibiting a yellowish hue, possibly indicative of an older stellar population. A faint, bluish disk extends outwards from the bulge, suggesting the presence of ongoing star formation activity within the disk. The disk appears relatively smooth, with limited observable distinct spiral arm structures. There is some visual evidence of a possible minor disturbance in the outer regions of the disk, potentially indicative of a past or ongoing interaction with another galaxy or infalling material. The galaxy's shape is highly elongated.
