The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a slightly brighter, concentrated core. The overall color profile suggests a redder population, indicative of older stars and potentially lower levels of ongoing star formation. There is no apparent disk structure, spiral arms, or significant dust lanes visible in this image, supporting a classification towards the elliptical end of the Hubble sequence. There also do not appear to be any major disturbances or mergers currently occurring with the galaxy. The round profile suggests a fairly relaxed system. The half-light radius appears to be relatively compact.