The galaxy presents as a relatively smooth and rounded structure with a concentrated central region. There is no clear evidence of spiral arms or a prominent disk. The light distribution appears centrally concentrated, fading gradually outwards with a smooth profile. The color is biased toward the blue end of the spectrum, suggesting a population of younger, hotter stars contributing to the overall light output. There appear to be no signs of significant tidal disturbances or ongoing mergers, based on the lack of morphological distortions or asymmetric features. Overall, the galaxy appears to be a fairly typical, undisturbed elliptical galaxy in a relatively early stage of its evolution.
