The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, fading gradually outwards. The core exhibits a reddish hue, possibly indicating an older stellar population, while the outer regions show a transition to a bluer color, suggesting the presence of some younger stars, though star formation activity appears relatively low overall. The galaxy displays a slight elongation, deviating minimally from a perfectly circular shape. No signs of significant tidal disturbances, major mergers, or prominent disk structures are evident.
