This galaxy presents as a relatively small, edge-on disk galaxy. It exhibits a bright, well-defined central bulge, with a noticeable flattened disk extending outwards. The light from the galaxy is characterized by a color gradient, transitioning from bluer hues in the disk, suggesting active star formation, to redder hues in the central bulge, indicating an older stellar population. Faint, diffuse features are visible extending outward from the disk, potentially indicative of tidal interactions or minor disturbances. While the main structure appears relatively undisturbed, there are subtle asymmetries that may suggest a recent minor merger or interaction. Further spectroscopic analysis would be needed to ascertain the redshift, star formation rate, and chemical composition of this object.
