The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center in a bright nucleus, surrounded by a diffuse, less luminous halo that gradually fades into the background. The galaxy exhibits a relatively round shape, with no apparent strong distortions or tidal features indicative of a recent major merger event. There are subtle color gradients visible, with a tendency toward bluer tones near the core, possibly indicating ongoing star formation within the central region. Fainter reddish hues are observed in the outer regions, which may suggest an older stellar population and/or increased dust extinction. Although primarily smooth in appearance, there is a hint of possible minor disturbance or asymmetry in the outer isophotes, suggesting a possible minor interaction in its past. 
