The galaxy presents a largely smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a bright core that gradually fades outwards without distinct features such as spiral arms or a bar. Its overall shape is predominantly round, with a high degree of circular symmetry. There is little evidence of recent or ongoing major mergers or significant tidal disturbances. The galaxy exhibits a colour gradient, with a generally redder hue in the core transitioning to slightly bluer colours in the outer regions. This colour gradient suggests a mix of older stellar populations in the center, potentially with relatively low levels of ongoing star formation in the galaxy's outskirts. 
