The galaxy presents a predominantly smooth morphology, with a slight elongation along its major axis, suggesting an elliptical or lenticular classification. The central region exhibits a bright, concentrated nucleus, characterized by a yellowish-orange hue, possibly indicative of an older stellar population. Fainter bluish light surrounds the core, possibly suggesting the presence of a relatively younger stellar population outside of the core. No strong evidence of spiral arms or significant dust lanes is discernible. There is a very slight indication of a possible minor disturbance in the smoothness of the galaxy, but it appears mostly relaxed. The object displays a moderate apparent size and luminosity, consistent with a galaxy at intermediate redshift.
