The galaxy presents as an elliptical or lenticular type, exhibiting a centrally concentrated bulge surrounded by a less defined, fainter disk or halo. It has an apparent tilt, with its major axis extending approximately horizontally in the image. There is a clear decrease in luminosity moving outward from the center, which appears smooth, uniform in color, and very bright. The outer regions have a grainy texture and a faint, bluish hue, indicating the presence of a younger stellar population. Subtle deviations or disturbances may indicate minor gravitational interactions.
