The galaxy presents as a moderately luminous, elongated object with a smooth overall appearance. Its morphology leans towards a spheroidal shape, although a subtle, extended feature suggests a possible disk component. The primary color appears to be a yellow-orange hue, indicative of an older stellar population. The color suggests relatively low rates of current star formation, and that most stars are more evolved. There is no obvious evidence of active galactic nuclei activity or significant dust lanes. Overall, the galaxy appears as a mature system, possibly undergoing a transition from a more active, disk-dominated phase to a quiescent, elliptical form. The structure appears mostly undisturbed, with no major signs of recent mergers or tidal interactions. A slight asymmetry could indicate minor disturbance or a very minor merger in its past.
