The galaxy appears to be relatively small and compact, presenting an irregular morphology. A bright, concentrated central region is evident, possibly indicative of an active galactic nucleus or a dense stellar population. Surrounding the core, there's a less defined, somewhat amorphous structure with hints of a disk-like component. This surrounding area exhibits a mottled texture, suggesting patchy star formation or dust obscuration. A faint, extended halo or tidal feature might be present, although difficult to discern definitively. The color distribution shows a range from bluer hues near the central region, possibly signaling younger stars, to slightly redder tones in the outer areas, potentially representing older stellar populations or dust extinction. Overall, the galaxy's morphology suggests it may be undergoing some form of interaction or exhibiting internal disturbances, departing from a simple elliptical or spiral classification.
