The galaxy presents a generally smooth morphology, with a central bulge that exhibits a yellowish-white color, suggestive of an older stellar population. The outer regions of the galaxy appear more diffuse, exhibiting a bluer hue, hinting at the presence of younger stars and ongoing star formation. There is no prominent spiral arm structure or bar visible in the image. The shape of the galaxy appears to be generally round, with no obvious major disturbances or indications of ongoing merging events.
