The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated luminosity with a yellowish-orange hue, indicating an older stellar population. Moving outward from the core, the galaxy fades in intensity, displaying a more diffuse, bluish color. This suggests the presence of a younger, bluer stellar population in the outer regions, potentially regions of ongoing or recent star formation. The overall shape is slightly elongated but largely spheroidal. There appears to be no obvious spiral arm structure or bar feature. There is no apparent indication of a major merger event or strong tidal disturbances, though faint asymmetries cannot be ruled out with certainty.
