This galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical light distribution. There is a pronounced central bulge that appears more luminous, transitioning to a more diffuse halo. The core exhibits a yellowish hue, which could indicate an older stellar population dominating the central region. Fainter, bluer regions surround the central bulge, indicating some pockets of younger stars and possibly ongoing, but low, star formation. There is no evidence of spiral arms or a defined disk. The galaxy does not seem to be undergoing a major merger, although some minor asymmetrical disturbances may be present. Overall, the galaxy presents as relatively undisturbed and relaxed in form.
