The observed galaxy presents a notably smooth morphology, exhibiting a predominantly elliptical shape. There is no visual evidence of spiral arms or a prominent disk structure. The galaxy appears largely undisturbed, with minimal indication of ongoing or recent merger activity. The light profile suggests a centrally concentrated brightness distribution, fading gradually towards the outer regions. The galaxy appears relatively compact, with its luminosity concentrated in a small spatial extent. In general, its structural features suggest classification as an elliptical galaxy with little to no recent interactions.
