The galaxy presents as a luminous, elliptical structure with a smooth, concentrated morphology. There is a central bulge that appears bright, yellow, and densely packed with stars. Moving outwards from the center, the luminosity gradually decreases, fading into an extended, less defined halo. It appears that the galaxy is slightly elongated, but otherwise shows no obvious signs of disk-like features or spiral arms. There do not appear to be any tidal tails or prominent disturbances in its shape, implying no recent major merger activity. The galaxy has a redder color, which suggests an older stellar population and a relatively low rate of ongoing star formation.
