The galaxy presents as a moderately bright object, exhibiting an overall elliptical morphology. The light distribution appears relatively smooth, with a centrally concentrated region of higher intensity. The color profile is slightly redder, suggesting a population of older stars dominates the stellar content. There are no distinct spiral arm features or dust lanes visible. The overall impression is that of a relatively undisturbed, evolved system. There is a very subtle suggestion of a possible minor disturbance.
