The galaxy presents a generally smooth morphology, with a high degree of central concentration. The overall shape is neither perfectly spherical nor significantly elongated. Instead, the form sits between a perfectly round and cigar-shaped structure. There is a small amount of evidence to show a disk, but the main portion of the galaxy looks smooth. The galaxy exhibits a color gradient, appearing bluer in the outer regions and transitioning to a redder hue closer to the core, which is suggestive of an older stellar population. The galaxy appears undisturbed, with no visible signs of ongoing or recent major merger events. Based on the observed color profile and morphology, the galaxy is likely a massive system, with an estimated stellar mass slightly above 10^10 solar masses. Star formation appears to be subdued, with a modest SFR and extremely low specific star formation rate. 