The galaxy presents as a flattened spheroid, with an apparent disk-like structure. Its central region exhibits a concentrated luminosity gradient, suggesting a prominent bulge. The overall color profile indicates a redder core transitioning to bluer hues in the outer regions of the disk. The smoothness of light distribution suggests minimal clumpy structure, possibly indicating a relatively evolved stellar population. Evident is a slight asymmetry of the galaxy indicating a probable recent interaction with another galaxy. The outer regions of the galaxy are indistinct and show possible signs of disruption.
