The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a notable central bulge with a high concentration of light. This bulge displays a yellowish hue, potentially indicative of an older stellar population. Surrounding the central region is a fainter, more diffuse halo or disk-like structure that extends outwards. This outer region shows some hint of a reddish color, possibly indicating the presence of dust or a slightly younger stellar population compared to the bulge. The galaxy appears somewhat elongated, but generally lacks any signs of significant spiral arm structures or major morphological disturbances. This suggests it has undergone significant merging in its history. Overall, the galaxy presents a relatively quiescent appearance.
