The galaxy presents a largely smooth, elliptical morphology, appearing quite rounded in shape. There's a notable concentration of light towards the center, indicating a prominent galactic nucleus. A relatively uniform color distribution across the galaxy suggests an older stellar population, with potentially limited ongoing star formation. There is no clear indication of distinct spiral arms or bar structures. No major merger events appear to be in progress, though subtle disturbances might be present. The galaxy's overall smooth appearance indicates it may be a relatively evolved system.
