The galaxy presents as a centrally concentrated, elliptical structure. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the color transitions into a more diffuse and slightly bluer halo. This suggests the presence of a younger stellar population or recent star formation in the outer regions, albeit at a subdued level. The galaxy appears relatively smooth with no discernible spiral arm structure or major morphological disturbances. There is a slight elongation visible in the overall shape, moving towards the "cigar shape" end of the spectrum, but it is primarily elliptical. Faint hints of tidal features are apparent on one side, possibly hinting at a minor interaction with a smaller galaxy. However, the main body of the galaxy remains largely undisturbed, signifying the absence of any ongoing major merger events.
