The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is a slight flattening of the galaxy, hinting at a possible disk component, but it is not well-defined. The color appears to be yellowish-orange, which could indicate an older stellar population with less ongoing star formation. There are no obvious signs of recent major mergers or tidal disturbances in the main body of the galaxy, although a very slight asymmetry might be present. Overall, the galaxy has an undisturbed appearance.
