The galaxy presents as a largely featureless, elliptical object. Its core exhibits a bright, yellowish-white hue, suggesting a high concentration of older stellar populations. The light gradually diffuses outward, transitioning to a slightly reddish-orange color in the outer regions. This color shift may indicate a decreasing density of younger, bluer stars and a predominance of cooler, redder stars in the galactic outskirts. The galaxy's morphology appears smooth and regular, with no apparent signs of ongoing mergers or significant tidal disturbances. There is minimal evidence of prominent spiral arms or a distinct disk structure. The overall impression is of a relatively quiescent galaxy with a well-mixed stellar population and a spheroidal shape.
