The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, emitting more light in the redder wavelengths. There's minimal evidence of spiral arms or significant dust lanes within the visible structure. The overall shape is slightly elongated, deviating marginally from a perfect circle. Hints of faint extended emission are visible around the central core. The galaxy's structure does not indicate any major ongoing merger events, although there may be a minor disturbance or interaction affecting its shape. Star formation rate appears relatively low, consistent with an evolved stellar population. 
