The galaxy presents as an elliptical system with a smooth, relatively featureless morphology. The light profile suggests a high degree of central concentration with a significant fraction of the overall light emanating from the core region. There is little evidence of spiral arms, dust lanes, or prominent star-forming regions. The galaxy appears to be relatively undisturbed, exhibiting a high degree of rotational symmetry. A faint, diffuse halo may extend beyond the main body of the galaxy, however this is difficult to discern with certainty. A faint neighboring galaxy is visible nearby. The galaxy's color index indicates a population of older, redder stars, which is consistent with the lack of active star formation and the smooth morphology. The galaxy is relatively massive. Overall, the characteristics suggest a passively evolving elliptical galaxy located at a considerable distance.
