The galaxy presents a somewhat smooth morphology with a slight central concentration of light. It appears relatively rounded in shape, with a lack of significant visible features such as spiral arms or a bar structure. There is a hint of a possible tidal tail or minor disturbance on one side, suggesting a past or ongoing interaction with another galaxy, but further investigation is required to confirm this. Color gradients within the galaxy are subtle, but there appears to be a bluer core than outer regions, possibly signifying on-going star formation. Overall, the galaxy seems to be relatively isolated and undisturbed, with a dominant spheroidal component. 
