The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish hue, suggesting an older stellar population. There's a subtle falloff in intensity from the center outwards. The outer regions display a slight greenish tint, potentially indicating a lower density of older stars or the presence of some younger, bluer stellar populations, although these are not distinctly resolved. There's a lack of any obvious spiral arm structure or irregular features; the overall structure is quite symmetrical. The galaxy appears relatively isolated, showing no significant signs of interaction or merging events based on the image data. It is moderately sized, but appears relatively compact. 
