The galaxy presents as a generally smooth structure, likely elliptical or lenticular. A subtle disk-like component is suggested by a slight flattening of the overall shape. The central region exhibits a concentration of light, indicating a nucleus or bulge. Color gradients are subtle, with a slightly redder hue towards the central regions, possibly indicating an older stellar population. Overall, the galaxy does not show obvious signs of significant disturbances or ongoing major mergers, although a hint of asymmetry could suggest minor interactions. The light distribution indicates it is not perfectly circular, leaning more towards an in-between elliptical shape.
