This galaxy presents as a centrally concentrated, elliptical-like structure. The light distribution appears relatively smooth and uniform, with a diffuse, extended halo surrounding a brighter, more compact core. The color profile exhibits a redder hue centrally, transitioning towards a slightly bluer tint in the outer regions of the halo, suggesting potential differences in stellar populations and ongoing star formation activity in those areas. No distinct features such as spiral arms or prominent dust lanes are discernible in this observation. There is no evidence of major disturbances or ongoing merging events.
