The galaxy presents an overall smooth morphology, with a possible disk-like structure evident at one end. The central region appears more concentrated and exhibits a reddish hue, suggestive of an older stellar population and potentially a larger bulge. The outer regions show a bluer coloration, indicating the presence of younger, hotter stars and active star formation. There are hints of some minor distortions or disturbances in the galaxy's structure, although no clear signs of major mergers are apparent. The galaxy appears elongated, with a shape that can be characterized as being between round and cigar-shaped. 
