The galaxy presents as a centrally concentrated object, exhibiting a somewhat elliptical morphology. It is characterized by a diffuse, extended halo surrounding a brighter, more compact core. The color profile suggests a mixed stellar population. The core appears to be bluer, potentially indicating ongoing or recent star formation activity. Fainter, redder light is observed in the outer regions of the galaxy. Irregularities within the galaxy's structure are mild, perhaps suggestive of minor gravitational interaction or internal dynamical processes. Overall, the galaxy gives the impression of a system transitioning from a more actively star-forming phase to one dominated by an older stellar population.
