The galaxy presents a somewhat elongated, elliptical morphology. Its light profile appears smooth and relatively featureless, with no prominent spiral arms or distinct dust lanes visible. There is a subtle color gradient, transitioning from a more yellow-red hue in the central regions to a slightly bluer tinge towards the outer edges. This could indicate an older stellar population concentrated towards the center, with younger, bluer stars forming in the outer regions. The galaxy seems relatively isolated, with no obvious signs of recent major mergers or tidal interactions that drastically affect its overall structure, however there is a slight irregular shape indicating possibly a minor disturbance from another galaxy.
