The galaxy presents an elliptical morphology, with a smooth, symmetrical appearance. The central region exhibits a concentrated luminosity, gradually decreasing towards the outer edges. The color profile suggests a dominant population of older stars, indicated by the reddish-orange hue, with some evidence of intermediate-age stellar populations showing a green tint. There is some slight asymmetry visible, and a possible indication of disk features, warranting further investigation into potential tidal interactions or internal structures. There appears to be minimal dust extinction. There are no prominent spiral arms or other distinct features associated with active star formation visible in this image.
