This galaxy presents as an elliptical or lenticular type. It exhibits a smooth, diffuse light profile suggesting an older stellar population. The core region is notably brighter and more concentrated than the outer edges, with a smooth transition in luminosity. There is little evidence of spiral arms or active star formation regions within the galaxy's structure. Its shape is elongated, indicating a moderate degree of ellipticity, although it does not appear severely distorted, exhibiting a primarily undisturbed morphology. Color gradients suggest a redder hue overall, consistent with aging stellar populations, with a slightly bluer tint near the center. No prominent dust lanes or signs of ongoing mergers are immediately apparent from the image.
