The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a notable lack of distinct spiral arms or a well-defined disk structure. The color profile suggests an older stellar population, with a dominant yellowish-red hue indicative of evolved stars and a low rate of on-going star formation. There are no prominent dust lanes or regions of intense blue star formation visible. The galaxy's surface brightness gradually decreases from the core outwards, indicating a relatively homogenous distribution of stars. There is no visual evidence of any recent major mergers or significant tidal disturbances affecting its overall structure.
