The galaxy presents a generally elliptical morphology. There is evidence of a central bulge, exhibiting a yellowish hue, with a more diffuse and bluer disk extending around it. The disk appears relatively smooth, lacking any prominent spiral arm structure. The galaxy shows a modest amount of star formation. There are no obvious signs of major mergers, although the presence of some morphological disturbances cannot be ruled out. The galaxy has a moderate mass. Overall, the galaxy seems to be a relatively isolated system undergoing moderate star formation.
