The galaxy appears as a relatively smooth, elliptical-like structure. There's a bright central bulge that dominates the overall luminosity, with the light appearing to fade gradually outwards into the surrounding halo. The color profile suggests an older stellar population, with a yellowish-red hue indicating a lack of significant ongoing star formation. There is some evidence of a faint, extended disk. Based on its apparent shape and color, it can be suggested that this is likely a fairly massive galaxy, with the data provided suggesting it is a relatively non-star-forming galaxy. It does not seem to be undergoing any major merger activity and shows no signs of strong tidal disturbances.
