The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears elliptical, with no immediately discernible spiral arms or distinct features. The core exhibits a brighter, more condensed region, likely a galactic bulge. The color distribution suggests a mixed stellar population. The central region appears bluer, possibly indicative of younger stars or ongoing star formation, while the outer regions seem redder, potentially composed of older, cooler stars. There is a slight asymmetry in the extended halo, possibly suggesting a minor interaction or disturbance in the past, but this is not readily obvious. Overall, the galaxy appears as a moderately luminous, elliptical galaxy with a hint of recent star formation activity in its core.
