The galaxy presents a somewhat elongated, elliptical morphology. The central region exhibits a high degree of luminosity, appearing as a bright, concentrated core. Moving outward from the core, the luminosity gradually decreases, with a smoother transition towards the edges.  There appears to be some disk structure to the galaxy as well.

Color gradients are subtle, with the central bulge exhibiting a slightly yellower hue, potentially indicating an older stellar population. The outer regions appear somewhat bluer. Overall the light is smooth and even, with little evidence of distinct spiral arms. The light distribution suggests the galaxy may be inclined relative to our line of sight. There may be a faint dust lane or other obscuring material present.

