This galaxy presents as a relatively smooth, rounded structure with a bright central core. There is a general absence of distinct spiral arms or prominent disk features. The light distribution appears concentrated towards the center, suggesting a high degree of central luminosity. The color profile indicates a mixture of stellar populations, with hints of bluer regions perhaps indicating ongoing star formation, though the dominant color is consistent with an older stellar population. There is a subtle suggestion of minor disturbances in the outer regions, though these do not dramatically alter the overall symmetric morphology.
