The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. Its color profile suggests an older stellar population, with a noticeable absence of distinct blue star-forming regions. The light appears yellowish-white, indicative of a population of evolved stars. There is no discernable spiral structure or prominent dust lane. The galaxy is relatively undisturbed, showing no clear signs of ongoing or recent major mergers or tidal interactions. A faint, extended halo is visible, gradually fading into the background. Overall, the galaxy appears to be a relatively massive, evolved system, potentially quiescent in its star formation activity.
