The observed galaxy presents a morphology that deviates from a simple elliptical or spiral classification. The central region exhibits a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. This core appears to be surrounded by a complex structure, with hints of possible tidal features or disrupted arms extending outwards.

The color distribution across the galaxy is not uniform. The central core has a significantly bluer hue, suggesting ongoing star formation or a population of hot, young stars. The outer regions exhibit a redder color, potentially indicating an older stellar population or the presence of dust obscuring bluer light. The general structure seems to show a possible interaction or merger event, as the overall shape of the galaxy is quite irregular. Evidence for disturbance is noticed, but it is not severe.
