The galaxy presents a somewhat irregular morphology, appearing as a generally elliptical object with a notable extension or arm-like feature on one side. The central region exhibits a bright, concentrated core, possibly indicative of a central bulge or active galactic nucleus. The galaxy displays a color gradient, with the core tending toward bluer hues and the outer regions showing redder tones. Patches of enhanced blue emission are visible in the core, which could be indicative of active star formation regions, while the redder extended feature may indicate a more aged stellar population and higher dust content. Overall, the structure suggests a galaxy that has potentially undergone some interaction or merger event, leading to morphological disturbances, or is actively in the process of forming stars in its central regions. The apparent smoothness indicates a evolved system with a minor bulge and/or disk component.
