The galaxy presents as a largely smooth, elliptical-like structure, exhibiting a centrally concentrated luminosity profile. The core region is characterized by a bright, yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the galaxy appears to transition to a bluer color, possibly indicating the presence of younger stars. The overall shape is more rounded than elongated. There is no strong evidence of spiral arms or a well-defined disk structure. There does not appear to be any major merging activity or significant tidal disturbances affecting the morphology.
