The galaxy presents as a singular, extended object with an overall smooth appearance. There is a subtle color gradient evident, with a central region exhibiting a more yellowish-orange hue suggestive of an older stellar population. This central region appears to be composed of two distinct, yet closely associated, high surface brightness knots or clumps. The outer regions of the galaxy fade into a fainter, more diffuse halo or envelope. There is a very slight hint of asymmetry, with one side appearing more extended. The morphology suggests either a possible early-stage merger event or significant internal disturbance within the galaxy's structure. The lack of clear spiral arms or distinct disk features supports the interpretation of a spheroidal or elliptical morphology, possibly undergoing transformation. Star formation appears low.
