This galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated brightness profile that gradually fades towards the outer regions. The core is a bright, yellowish-white hue, suggesting a population of older stars. The outer regions appear slightly bluer, which could indicate the presence of some younger stellar populations, although this is not particularly prominent. There is no evidence of significant spiral structure, or tidal disturbances, indicating that the galaxy is likely not undergoing any major merging events. The galaxy appears mostly round in shape.
