The galaxy presents a generally smooth morphology, with a slight elongation suggesting an elliptical or lenticular classification. Its light profile exhibits a concentrated central bulge, transitioning smoothly outwards into a more diffuse halo. Color gradients are subtle, with the core appearing slightly yellower, possibly indicating an older stellar population, and the outer regions exhibiting a bluer hue, potentially due to younger stars or recent star formation, though this activity appears relatively subdued. There is no prominent spiral structure, suggesting a lack of significant ongoing merger activity or dynamic instability. Faint hints of tidal features or minor disturbances cannot be ruled out. Overall, it appears to be a relatively evolved system, though further spectral data would be needed for a more robust characterization of its stellar populations and star formation history.
