The object appears to be a spiral galaxy viewed edge-on. The prominent central bulge is distinctly elongated along the major axis of the galaxy. The bulge displays a smooth, rounded morphology. A faint disk is visible, extending outwards from the central bulge. There is no immediately apparent sign of dust lanes within the disk. No signs of recent or ongoing major mergers, strong tidal disturbances, or prominent star formation regions are observed. The galaxy has a red hue, indicating a lack of active star formation, and therefore a relatively older stellar population. The overall shape is relatively symmetrical.
