The galaxy presents a generally smooth appearance with a centrally concentrated bulge that dominates its overall structure. The light from the galaxy exhibits a radial gradient, brightest at the core and gradually fading outwards. The core displays a yellow-orange hue, suggesting an older stellar population and reduced star formation in this central region. The outer regions of the galaxy appear slightly bluer, possibly indicating some ongoing or recent star formation, albeit at a lower rate. The galaxy's shape is somewhat elongated, although not significantly so, showing that it is not entirely spherical, but instead somewhere in between round and cigar-shaped. There is no obvious indication of spiral arms or a distinct disk component; it lacks strong features indicative of merging or tidal disturbances.
