The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge region that dominates the light profile. Moving outward from the core, the luminosity gradually decreases, exhibiting a diffuse halo. Faint color variations are present within the galaxy, suggesting a range of stellar populations. A subtle dust lane or disturbance may be present, indicating a possible minor interaction or recent accretion event. The overall structure appears relatively undisturbed, lacking prominent spiral arms or significant irregular features. The galaxy’s color indices suggest a population dominated by older stars with moderate ongoing star formation.
