The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse morphology with a concentrated central bulge. The color profile indicates a dominant population of older stars, with the core of the galaxy displaying a yellow-orange hue. Fainter, bluer regions are discernible, indicating the presence of some younger stellar populations. There is a slight asymmetry to the outer regions. There is no evidence of spiral arms or a prominent disk structure within the resolution limits of the image.
