The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. Its overall shape is elliptical, exhibiting a high degree of roundness, with only a slight deviation towards an elongated or cigar-like form. The central region displays a brighter, yellowish-orange hue, which may indicate an older stellar population. The outer regions of the galaxy become fainter, showing a bluer tint, hinting at the presence of some younger stars. There is no evidence of prominent spiral arms or strong tidal disturbances. No signs of an ongoing or recent major merger are apparent. The overall light profile suggests a well-established, stable galactic structure.