The galaxy presents as a somewhat smooth, elliptical object with a concentrated central bulge. There's a slight elongation, suggesting a deviation from perfect sphericity. The color appears predominantly yellow-white, indicating a stellar population dominated by older, less massive stars, although a hint of bluer regions suggests some ongoing, albeit limited, star formation activity. No distinct spiral arms or significant dust lanes are discernible, further supporting a classification toward the elliptical end of the Hubble sequence. There is a very subtle disturbance in the morphology that indicates a possible minor merger event in its past or even ongoing.
