The galaxy appears as a somewhat elliptical, centrally concentrated object. The core region exhibits high luminosity, gradually decreasing in intensity outwards. The overall color profile suggests a mature stellar population, dominated by older, redder stars with a hint of yellow in the central bulge. There is no discernable spiral structure or significant dust lanes visible in this image. The galaxy presents a smooth, relatively undisturbed morphology, with only a very slight asymmetry suggesting a possible past minor interaction. The dimensions indicate this is a moderately sized galaxy. The lack of intense blue regions indicates a low current star formation rate.
