The galaxy presents as a single dominant spheroid structure, exhibiting a smooth, concentrated luminosity profile. It appears largely elliptical in shape, with a high degree of roundness and no readily discernible spiral arms or bar structures. The core region shows a higher intensity, suggesting a concentration of older stellar populations. The galaxy's color index indicates a redder hue, which is consistent with a population of evolved stars and minimal on-going star formation. There are some signs that it could be merging with another galaxy, or otherwise experiencing some major disturbance.
