The galaxy presents as a smooth, elliptical structure with a high degree of central concentration. The light profile suggests a centrally dominant bulge component with a gradual decline in surface brightness towards the outer regions. The morphology exhibits a lack of spiral arms or distinct disk features. The galaxy's overall shape is somewhat elongated, but not significantly cigar-shaped. There is no readily apparent evidence of ongoing major merger activity or strong tidal disturbances. The dominant color is a yellow-orange hue, potentially indicative of an older stellar population, though a small component of recent star formation cannot be ruled out. 
