The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated luminosity, appearing yellowish-orange, suggestive of an older stellar population. Moving outwards from the core, there's a gradual decrease in surface brightness. The color shifts towards bluer hues in the outer regions, potentially indicating the presence of younger, hotter stars, or perhaps some ongoing low-level star formation. There may be a subtle hint of a disk-like structure, viewed nearly edge-on. The overall shape is elongated, appearing cigar-shaped with no obvious signs of major disturbances, although a minor interaction or disturbance cannot be entirely ruled out.
