The galaxy presents as an elliptical morphology, nearly spherical in shape, though potentially with a slight elongation along its major axis. Its core exhibits a bright, concentrated luminosity, indicating a high density of stars. The color gradient transitions from a yellowish-white core to a reddish-orange outer region, suggesting an older stellar population overall and potential differences in metallicity and stellar age between the core and periphery. No distinct spiral arms or significant dust lanes are readily apparent in this image, supporting its classification as an elliptical galaxy. There is a lack of blue light in the galaxy which would indicate the presence of younger stars and thus more star formation. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent major mergers or tidal disturbances.
