The galaxy presents as a relatively compact, centrally concentrated object. Its morphology appears largely smooth with a noticeable degree of central concentration. There is some indication of faint, diffuse structure extending outward from the core. It is round in shape and possesses a moderate redshift, indicating a significant distance. Based on its color indices, the galaxy exhibits a reddish hue, suggesting a relatively older stellar population with minimal ongoing star formation. There is no clear evidence of strong spiral arm structure or significant dust lanes. There is some indication of a small chance it is undergoing a merger.
