The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. There is a central bulge that appears more concentrated and exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy fade into a more diffuse halo, displaying a bluer tint, which might signify the presence of younger, hotter stars in the outskirts.

The overall shape is more 'in between' round and cigar shaped with a relatively high probability of not undergoing a major merger event currently or recently.
