The galaxy presents an elliptical morphology, appearing elongated in shape with a high degree of oblateness. The light distribution suggests a smooth profile, exhibiting a concentration towards the center. The color gradient is minimal, trending towards redder hues from its core outwards. A lack of prominent spiral arms or distinct dust lanes is noted. No indications of significant tidal interactions or major mergers are directly apparent. Close inspection may reveal a slight disturbance on one side of the object, but more investigation is required.
