The galaxy presents as a disk-shaped object, viewed nearly edge-on. There is an elongated, somewhat diffuse central bulge. The overall light distribution suggests a higher concentration towards the center, gradually fading into the outer regions of the disk. The galaxy exhibits a predominantly blue hue, suggestive of recent or ongoing star formation. The disk appears relatively smooth, with no obvious spiral arm structures visible at this resolution. Some areas of the disk also show a slightly bluer tint that suggests younger star formation and star clusters. Dust lanes appear to be only lightly distributed along the disk, due to the galaxy's color. The galaxy shows no prominent signs of interaction or merging.
