The galaxy presents as a slightly elongated, elliptical morphology. Its core exhibits a concentrated, yellowish hue, suggesting a significant population of older stars. The outer regions of the galaxy display a gradual decrease in luminosity and a transition toward redder tones. There is an apparent lack of distinct spiral arm structures or prominent dust lanes. The overall smooth appearance of the galaxy suggests a relatively quiescent state with limited ongoing star formation. There is little to no visual evidence of any tidal disturbances or major mergers, though there does appear to be some minor structure or interactions. 
