The galaxy presents as a somewhat smooth, elliptical object. The main body exhibits a concentrated, rounded central bulge with a diffuse halo extending outwards. The color profile suggests a dominant population of older stars, with a yellow-red hue throughout the primary structure. There appears to be a fainter, smaller region offset from the main body. This may indicate a minor tidal disturbance or a possible interaction with a smaller companion galaxy. There are no clearly defined spiral arms or prominent dust lanes visible in this image. Overall, the morphology suggests a galaxy with an evolved stellar population, potentially undergoing or having undergone a merger event.
