The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a subtle elongation of the galaxy, possibly indicating a slight deviation from a perfectly spherical shape. The light distribution suggests a dominant, centrally concentrated bulge. The galaxy exhibits a color gradient, appearing bluer in its central regions and gradually becoming redder towards the outskirts. This color gradient may be indicative of a difference in stellar populations, with younger, bluer stars concentrated in the center and older, redder stars populating the outer regions. There is no evidence of spiral arms or significant dust lanes. Faint tidal features or signs of recent mergers are absent, suggesting a relatively quiescent evolutionary history.
