The galaxy presents as a fairly smooth, elliptical-like structure with a prominent bulge. It has a moderately elliptical shape, appearing neither perfectly spherical nor strongly elongated. The galaxy's core exhibits a yellowish hue, suggesting a population of older stars. The outer regions display a bluer tint, potentially indicating ongoing or recent star formation, although this is more subtle. No significant dust lanes or distinct spiral arm structures are discernible in the image. There may be a very minor disturbance in the shape of the galaxy, suggesting a possible interaction with another galaxy in the past, or a very small, currently ongoing merger.
