The galaxy presents a roughly elliptical morphology, though significantly elongated. It exhibits a smooth overall appearance, suggesting a lack of prominent spiral arms or other distinct features. The color profile shifts from a bright, yellowish-white core region to a more reddish hue at the outer edges, hinting at varying stellar populations or dust distribution. Its elongated shape may be indicative of a spheroidal galaxy or potentially a disk galaxy viewed at a high inclination. There appears to be no strong signs of active galactic nuclei activity or significant star formation. It does not seem to be undergoing major mergers or significant tidal disturbances.
