The galaxy presents as a largely elliptical or spheroidal structure, with a relatively smooth light distribution. The core region exhibits a concentrated brightness, appearing more yellow in color, suggesting a population of older stars. A slight extension of light is visible beyond the bright central region. There appears to be some slight unevenness in the overall distribution of the galaxy's light, though no distinct spiral arms or significant dust lanes are apparent. The galaxy appears relatively isolated, with no clear signs of ongoing major merger activity or strong tidal interactions. There's also a slight bluish haze emanating from a small portion. The general morphology indicates a galaxy with a high degree of symmetry.
