The galaxy presents as a single, somewhat elongated, luminous entity exhibiting a smooth, diffuse morphology. The light distribution suggests a high degree of central concentration, with a gradual decline in intensity towards the outer regions. The overall color profile is indicative of an evolved stellar population, presenting as reddish-yellow hues. The apparent smoothness suggests it is likely an elliptical galaxy with little to no active star formation. There is a slight elongation, perhaps indicating a transition between elliptical classifications. The disk-like appearance could be the result of a merger, but further observations would be required. No prominent dust lanes or spiral arm structures are discernible within this limited data.
