The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The overall color profile suggests an older stellar population, with a yellowish-white hue dominating the central region, possibly indicative of evolved stars. A slight bluer tinge is observable in the outer regions, hinting at some ongoing, albeit low, star formation. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances, although subtle asymmetries or minor disturbances cannot be ruled out. The shape of the galaxy is tending towards round rather than cigar shaped. The size of the galaxy appears moderate. Overall, it likely constitutes a quiescent galaxy, with a substantial stellar mass.
