The galaxy presents as a smooth, elliptical-like structure. The central region exhibits a bright, concentrated light, suggestive of an older stellar population. Moving outward from the center, the light becomes less intense and the color reddens somewhat, indicating a wider distribution of evolved stars. There is a slight asymmetry to its shape. There is no distinct spiral arm structure or evidence of significant dust lanes visible in this image. The galaxy appears to be in a relatively quiescent state, without major disturbances. Overall, it shows the characteristics of a massive galaxy with a high likelihood of a well-established stellar population.
