This galaxy exhibits characteristics of a spiral galaxy viewed edge-on. There is a distinct central bulge that appears moderately concentrated, which is observed to be brighter and more uniform in color than the surrounding disk. This bulge fades smoothly into the disk. The disk is composed of a mix of colors, with hints of dust lanes and possibly some spiral arm structure. The disk is moderately asymmetric, indicating a possible minor disturbance due to tidal interactions or past mergers. The galaxy's overall profile suggests a significant portion of the stellar population is in the disk, with a noticeable dust obscuration along the galactic plane. The galaxy exhibits relatively low star formation activity. It contains a substantial stellar mass.
