The galaxy appears to be an elliptical galaxy, with a smooth, featureless morphology. Its overall shape is elongated, more akin to a cigar than a perfect sphere. The light profile suggests a concentrated nucleus, with the luminosity decreasing gradually outwards. The central region exhibits a yellowish-orange hue, indicating an older stellar population, potentially dominated by red giant stars. The outskirts show some hints of bluer light, possibly indicating some presence of younger stars but to a limited degree. There are no obvious signs of spiral arms, a prominent disk, or significant dust lanes. The galaxy is not showing strong indications of a major merger, although there might be minor disturbances present in the outer regions. The relatively smooth appearance indicates the galaxy has likely undergone significant dynamical relaxation.
