The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a gradual decline in brightness from the core outwards. The core itself is bright, suggesting a high density of stars, and appears yellowish-white in color, potentially indicating an older stellar population.  The outer regions of the galaxy exhibit a faint bluish color, possibly indicative of the presence of some younger stars or ongoing star formation, albeit at a low rate. The galaxy shows no obvious spiral arms, bars, or signs of major disturbances or tidal features. The shape is more akin to an elliptical than a spiral type. It exhibits only a slight deviation from a perfectly round shape. There are no apparent signs of a recent or ongoing major merger event.
