The galaxy presents as a relatively smooth, elliptical structure with a noticeable elongation. Its color profile suggests a dominant population of older stars, emitting more light in the redder wavelengths, with a general yellow hue. The core region appears brighter and more concentrated than the outer edges. There is no evidence of distinct spiral arms or dust lanes visible in this image, indicating a lack of significant recent star formation activity. The overall morphology is consistent with an elliptical galaxy.
