The galaxy appears as a somewhat elliptical, diffuse object. It exhibits a bright, concentrated central bulge that is slightly orange in color, suggesting an older stellar population. The surrounding disk shows a more greenish tint, potentially indicating the presence of younger, hotter stars and some star formation, but this is not prominent. The overall structure seems relatively smooth, with no distinct spiral arms or bar visible. There is no evidence of any major merger events or tidal disturbances in the image. The galaxy appears to be in a relatively quiescent state.
