The galaxy presents as an elliptical or spheroidal structure. Its morphology appears relatively smooth, lacking significant discernible features such as spiral arms or prominent dust lanes. The light distribution suggests a centrally concentrated brightness profile, with a gradual decrease in intensity towards the outer regions. Color gradients are subtle, with a slightly redder hue in the central region transitioning to a bluer tint in the outskirts, possibly indicating differing stellar populations. There are no obvious signs of ongoing major merging events or significant tidal disturbances. Based on these features, this galaxy likely represents a quiescent system characterized by a well-mixed stellar population and minimal active star formation within the last few Giga-years.
