The galaxy presents a predominantly smooth morphology, with a slightly elliptical shape. Its central region exhibits a bright, concentrated core indicative of a substantial stellar population or active galactic nucleus. The overall color appears relatively blue, suggesting the presence of ongoing or recent star formation. There is evidence of some minor disturbance in the disk but it seems to be mostly stable with no major distortions. There are some hints of spiral structure, but those hints may be due to minor disturbances. It is most likely not undergoing a major merger but may be experiencing some interaction with a small nearby galaxy.
