The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. There appears to be evidence of possible tidal distortions or interactions. The overall morphology indicates a relatively evolved system, likely with a dominant population of older stars. The galaxy exhibits a reddish-yellow hue, suggesting a lower rate of star formation. There is a significant amount of light emitted toward the center of the galaxy, making the core appear quite bright.
