The galaxy presents an overall elliptical morphology with a smooth light distribution. There is a notable concentration of light toward the center, suggesting a prominent galactic nucleus. The color profile indicates a redder hue overall. Based on the observed morphology and color, this galaxy is likely an elliptical galaxy composed of an older stellar population. The overall structure appears largely undisturbed, although there are slight irregularities in the luminosity profile that may indicate minor disturbances or past mergers. Star formation activity appears low.
