The galaxy presents a largely smooth and rounded morphology, exhibiting minimal features indicative of spiral arms or significant dust lanes. The overall light distribution appears centrally concentrated, with a gradual decrease in luminosity extending outwards from the core. Color gradients are subtle but noticeable, with the central region displaying a yellowish hue that transitions to a redder color in the outer regions. This suggests an older stellar population concentrated in the core, with potentially younger, bluer stars being less prominent. There is no indication of ongoing major mergers or tidal disturbances, though the possibility of minor interactions cannot be entirely ruled out based on this image alone. The galaxy presents an elliptical morphology overall, with a seemingly simple morphology, dominated by an ellipsoidal distribution of stars. 
