The galaxy presents a largely smooth and centrally concentrated morphology, with a high degree of circularity. The color profile suggests a dominant stellar population of older stars, as indicated by the redder hues observed. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy shows little evidence of recent or ongoing major merger activity, appearing largely undisturbed. Overall, the galaxy appears to be a relatively quiescent system, likely an elliptical galaxy with suppressed star formation.
