The galaxy presents as a relatively smooth and centrally concentrated object, exhibiting a predominantly elliptical morphology. The light profile gradually decreases from the core outwards, suggesting a lack of prominent spiral arms or a distinct disk structure. The core appears bright and slightly yellow, which may indicate an older stellar population dominating this region. The outer regions of the galaxy display a bluer hue than the core, which potentially points towards the presence of a younger stellar population and ongoing star formation within these regions. The overall symmetrical appearance suggests a relaxed dynamical state, with no obvious signs of major recent mergers or tidal disturbances. However, closer inspection reveals a slight asymmetry in the light distribution, perhaps hinting at a minor interaction or internal structure. The galaxy's moderate redshift suggests that it resides at a significant cosmological distance.
