The galaxy presents a relatively smooth morphology, with a dominant central bulge. The bulge exhibits a yellowish-red hue, possibly indicative of an older stellar population and/or dust obscuration. Extending outwards from the bulge, there is a hint of a disk-like structure, though it appears somewhat irregular or disturbed. Faint blue colors may indicate modest star formation. There is evidence for a possible merger event. This is based on what appears to be a tidal tail extending from the main body of the galaxy. The galaxy displays an intermediate roundness. The system's color suggests it is relatively mature, however the potential merger suggests ongoing interactions that could influence its future evolution.
