The galaxy presents as a smooth, elongated structure. It appears largely featureless, lacking prominent spiral arms or a well-defined central bulge. The galaxy exhibits a color gradient, transitioning from a yellowish core to bluer hues in the outer regions. This color variation suggests differing stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the periphery. The elongated shape is suggestive of an elliptical galaxy, potentially of type E6-E7, observed nearly edge-on. There is no obvious evidence of active galactic nuclei activity or significant dust lanes within the observed image. The galaxy does not show any obvious signs of major mergers or tidal disturbances.
