The galaxy presents as a relatively small, disk-shaped structure with a distinct central bulge. The disk appears to be oriented nearly edge-on from our perspective. The central bulge exhibits a smoother texture and appears to be more concentrated than the surrounding disk. Within the disk, I observe subtle indications of possible arm structures. There appears to be some disruption occurring that could be evidence of tidal disturbances, or perhaps minor interactions with another galaxy. The galaxy's color suggests it is likely in an active star-forming phase, with the presence of both young, hot stars and older stellar populations.
