The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The color profile indicates a dominance of older stellar populations, as evidenced by the reddish-yellow hue. There is a slight color gradient visible, with the central region exhibiting a more pronounced yellow tone, suggesting a higher concentration of older stars. The outer regions appear somewhat less concentrated and possibly bluer. The galaxy seems relatively undisturbed, displaying no significant signs of ongoing or recent merger activity, although some minor asymmetry in its halo might exist. It is highly likely to be a relatively massive galaxy with a low star formation rate. The overall shape is close to round.
