The galaxy presents an elongated morphology, potentially indicative of a spiral galaxy viewed edge-on or a lenticular galaxy. The light distribution appears relatively smooth, with a concentrated central bulge region exhibiting a brighter, more intense luminosity. There is a subtle suggestion of a disk component, with a more diffuse glow extending along the major axis. The overall color is predominantly greenish, possibly indicating active star formation or a specific stellar population. A faint, irregular structure appears in the bottom region of the galaxy, hinting at a possible tidal interaction or ongoing minor merging event. The absence of clearly defined spiral arms or prominent dust lanes suggests a relatively evolved system.
