The galaxy appears to be a relatively smooth, elliptical galaxy, likely at a significant distance given its apparent size. It displays a slightly elongated shape, approximating a cigar-like morphology. The light profile suggests a dominant bulge component with a smooth, diffuse halo. The color is predominantly yellow-orange, implying an older stellar population with fewer young, blue stars and relatively low ongoing star formation. There is no obvious evidence of spiral arms or a distinct disk component. No significant tidal disturbances or signs of ongoing major mergers are readily apparent. Overall, the galaxy is likely a quiescent, evolved system.
