The galaxy presents a largely smooth morphology, with a centrally concentrated light distribution. The color gradient suggests a population of older stars, exhibiting a yellow-red hue. There is a slight deviation from perfect circularity, suggesting a possible departure from a perfectly spherical shape. No distinct spiral arm structures or significant dust lanes are discernible, hinting at a relatively quiescent state of star formation. The galaxy appears generally undisturbed, lacking obvious signs of recent major mergers or tidal interactions.
