The galaxy presents a smooth, elliptical morphology. It exhibits a concentration of light toward the center, with a noticeable decrease in surface brightness as one moves outwards. The color profile suggests a relatively evolved stellar population, leaning towards redder wavelengths with subtle green hues in the outer regions. There is no apparent spiral structure or distinct dust lanes. The galaxy appears relatively isolated and undisturbed, displaying no obvious signs of recent major mergers or tidal interactions. Its elongated shape suggests a possible moderate degree of flattening.
