The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicative of a population of older stars. This bright central region gradually fades into a more diffuse halo. While there is no apparent spiral structure, some faint blue tones are present in the outer regions, suggesting the presence of some younger, hotter stars. These bluer regions appear patchy and not well-defined. There is no obvious dust lane or other distinct features, and the overall structure indicates minimal signs of recent interaction or merging events. The galaxy appears relatively isolated. Its size is significant, representing a notable mass, and while there is some star formation occurring, it is likely at a moderate rate.
