The galaxy presents a largely smooth, elliptical morphology. Its color profile shows a concentration of light in the redder wavelengths, with a decreasing presence of blue light, suggesting a population dominated by older stars. There is little to no evidence of spiral arm structure or significant dust lanes, reinforcing the classification of a relatively quiescent, early-type galaxy. A slightly elongated shape is observable. There might be some indications of a minor disturbance, though these are subdued. Overall, the galaxy appears to be an evolved system with a relatively low ongoing star formation rate.
