The galaxy presents as a relatively smooth, elongated structure. Its overall color appears yellowish-orange in the central region, transitioning to a bluish hue on the outer edges, potentially indicating younger stellar populations in the disk. The light distribution suggests a generally elliptical shape, with no obvious signs of spiral arms or significant morphological disturbances. The apparent lack of strong dust lanes further supports the observation of a relatively featureless, smooth galaxy. This could indicate a later-type galaxy, perhaps an elliptical or lenticular, with ongoing, but low, levels of star formation. The galaxy does not appear to be undergoing any major merging events with another galaxy, nor does it display any tidal tails or other significant signs of gravitational interaction.
