This galaxy presents as an elongated, cigar-shaped structure, likely an elliptical galaxy viewed from a significant angle. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, there is a subtle shift towards bluer tones in the peripheral regions, potentially indicating the presence of younger stars or ongoing, albeit limited, star formation. The galaxy appears relatively smooth in texture, with no prominent spiral arms or distinct morphological features. Slight disturbances can be seen on the edges of the light emmision. There is no evidence of a recent or ongoing major merger event from what is visible.
