This galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests it is likely an elliptical galaxy or a lenticular galaxy viewed at a shallow inclination. The galaxy exhibits a yellowish-white hue across the main body, potentially indicating an older stellar population with lower rates of star formation. There's no distinct spiral structure visible, and no clear evidence of a prominent dust lane or disk. The overall morphology points toward a spheroid-dominated system with minimal ongoing star formation, with some potential low levels of star formation. No significant signs of tidal disturbances or ongoing mergers can be seen in the image. The shape of the galaxy is in between being completely round and elongated but is leaning more towards round.
