The galaxy presents as a relatively smooth, elliptical morphology with a centrally concentrated luminosity profile. The central region exhibits a yellowish hue, suggesting a population of older stars. The outer regions of the galaxy fade gradually into the background, showing a smooth transition. There is a lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears somewhat flattened but is mostly rounded in shape. Minor irregularities or disturbances in the outer regions may indicate possible past interactions, however it has likely not undergone any major mergers. Overall, the galaxy appears to be relatively evolved and quiescent.
