This galaxy presents as a relatively bright, elongated object, likely a disk galaxy viewed nearly edge-on. The central region appears more concentrated and exhibits a yellowish-orange hue, suggesting an older stellar population and possible dust obscuration. Moving outwards from the center, the disk appears thinner and bluer in color. There appears to be some asymmetry in the disk, possibly caused by a minor gravitational disturbance or ongoing interaction. The overall morphology suggests a galaxy of moderate size and mass, exhibiting moderate levels of star formation activity, and likely has a relatively small bulge.
