The galaxy presents as a generally smooth and elliptical morphology, exhibiting a concentrated central bulge. There is a subtle gradient in the light distribution, with the core region appearing significantly brighter than the outer edges. The color profile suggests a population of older stars, appearing reddish-yellow, implying a relatively low rate of ongoing star formation. There are no prominent spiral arms, dust lanes, or distinct features indicative of recent mergers or active galactic nuclei activity visible in the image. The overall structure suggests a galaxy that is potentially in a state of relative quiescence.
