The galaxy presents as a smooth, elliptical structure. Its core exhibits a concentrated luminosity, appearing bright and slightly yellow. The light distribution suggests a relatively homogeneous stellar population throughout its central region. There is minimal evidence of spiral arms or significant disk features, supporting its elliptical classification. The overall roundness of the galaxy is apparent, though a subtle elongation is present. No major signs of ongoing mergers or significant disturbances are observed in the image. There may be some minor disturbances in the edges of the galaxy, but these are faint. Given its color profile, the galaxy is likely dominated by older stellar populations, with a suppressed rate of current star formation.
