The galaxy presents as a relatively smooth structure with a dominant, centrally located bulge. There are no obvious spiral arm features discernible. The object exhibits a roughly elliptical morphology, leaning towards a round shape. 

Evidence suggests a potential interaction or disturbance, exhibiting a minor irregularity in its form. The primary body of the galaxy displays a yellow hue, indicative of an older stellar population, with possible ongoing star formation in the central region giving off a slight greenish tinge. The galaxy shows no obvious signs of a major merger event, although a minor disturbance may be present. The galaxy's estimated size is approximately 5 kpc in radius, a reasonably compact structure.
