The galaxy presents as a somewhat diffuse object, exhibiting a generally elliptical morphology. Its core region appears brighter and more concentrated, displaying a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy appear less defined and more spread out, with hints of bluish light on the bottom, potentially indicating some ongoing star formation. Overall, it appears to be a relatively isolated galaxy, exhibiting no obvious signs of a major ongoing merger, but possibly some minor disturbances to its morphology.
