The galaxy appears to be a luminous, elliptical type, exhibiting a smooth, spheroidal morphology. The light distribution suggests a centrally concentrated structure with a gradual decrease in surface brightness outward. There is a marked absence of distinct spiral arms or a prominent disk component. The galaxy's color profile shows a yellowish hue centrally, transitioning to a redder tint in the outskirts. This color gradient could indicate an older stellar population dominating the central regions, while relatively younger, though still aged, stars may populate the outer reaches. There are no signs of significant tidal disturbances or ongoing mergers. The galaxy seems relatively undisturbed, suggesting a period of quiescence in its recent history.
