The galaxy appears as a centrally concentrated object, exhibiting a smooth and rounded morphology. The color profile suggests a significant population of older stars, with a noticeable absence of blue, indicating minimal ongoing star formation. There is no visible spiral structure or disk-like feature. Based on the faint disturbances, one might assume there is a chance of a very minor merger in the past but it would not be conclusive. The galaxy presents as an evolved system, likely an elliptical galaxy with a substantial stellar mass.
