The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a largely featureless morphology. Its overall shape is generally round. The galaxy presents a concentration of light towards its center, suggesting a prominent galactic nucleus. There is a subtle color gradient, trending from blue-white near the core to a more red-shifted hue in the outer regions. This could indicate a difference in stellar populations, with older, redder stars dominating the outer regions, and possibly ongoing star formation within the central area, although at a relatively low rate. There is no clear evidence of spiral arms, bars, or significant dust lanes. The galaxy does not appear to be undergoing any major merging events or showing signs of significant tidal disturbances.
