The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. There is a subtle elongation, though it mostly appears rounded. The galaxy displays a color gradient, transitioning from a redder core region to bluer outer regions, which may indicate ongoing or recent star formation activity, particularly in the outer regions. The galaxy appears relatively isolated, with no signs of ongoing major mergers, though a possible minor tidal disturbance or a faint companion galaxy may be present. The dominant light is concentrated towards the center, indicating a high concentration of older stars in the core.
