The galaxy presents a generally smooth, elliptical morphology. It appears relatively round. Its color profile leans towards the redder end of the spectrum, with a pronounced yellowish hue indicating an older stellar population and minimal ongoing star formation. There is no discernible disk structure or spiral arms. The galaxy's light profile suggests a concentrated core with a gradual decrease in luminosity towards its outer regions. The galaxy appears largely undisturbed, showing no major signs of mergers or tidal distortions, though some minor asymmetries could suggest past interactions.
