The galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent central bulge dominates the structure, appearing yellowish-orange, likely indicating an older stellar population. A faint, elongated disk extends from the bulge, also displaying a generally smooth texture. The disk appears relatively thin, with a subtle dust lane perhaps visible. The absence of clearly resolved star-forming regions or spiral arm structures further suggests a lower rate of current star formation. The smooth appearance of the galaxy hints at a possible history of recent mergers, though no distinct tidal tails or distorted shapes are observable.
