This galaxy presents as an elliptical morphology, showing a smooth, concentrated light profile that suggests an older stellar population. The central region exhibits a yellowish hue, indicative of evolved stars. Moving outward from the core, the galaxy's color transitions to a slightly bluer tone, hinting at the presence of younger stars, though their contribution appears minimal. The galaxy's overall shape is elongated, and shows hints of a slight disk-like structure. There are no prominent dust lanes or spiral arm features visible. The galaxy is appears to be relatively undisturbed, lacking signs of major tidal interactions or recent merger events. A minor perturbation cannot be excluded. The limited color variation suggests that the current star formation rate is suppressed.
