The galaxy presents as a generally smooth, centrally concentrated object with a somewhat round morphology. Its color profile exhibits a gradient from a brighter, yellower core to a slightly fainter, redder outer region. There is no apparent spiral structure or disk component visible. No significant tidal features or signs of a major merger are evident. Subtle irregularities in the outer halo suggest minor gravitational disturbances or past interactions, but these are not pronounced. The galaxy appears relatively isolated.
