The galaxy presents as a relatively smooth, elliptical-like structure, with no apparent spiral arms or significant dust lanes visible in this imaging. The central bulge region is quite prominent and appears to be a yellow or white hue, suggesting an older stellar population. The overall color of the galaxy shifts towards a bluer tint on the outskirts, indicating the potential for some ongoing, albeit limited, star formation in the outer regions. The galaxy appears to have an approximate effective radius of 7 kpc. There are no obvious signs of major tidal disturbances or ongoing mergers, though the irregular shape hints at a possible minor interaction. Overall, this galaxy exhibits characteristics consistent with an elliptical galaxy that has largely ceased active star formation, but not entirely.
