The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a high degree of concentration, indicated by the brighter, yellowish core. The light gradually decreases in intensity outwards from the center, with no apparent spiral arm structures or significant dust lanes visible. The overall shape appears roughly rounded, transitioning to a slightly more elongated form at its periphery. There is no clear evidence of major disturbances or ongoing merger activity. The galaxy's color profile suggests a population of older stars, with redder hues dominating. Star formation appears to be suppressed. 
