The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. The color profile suggests an older stellar population, indicated by the yellow-red hue towards the core. Fainter, bluer regions are observed on the outer edges suggesting some star formation is present, although low. The galaxy exhibits a high degree of circularity. No significant signs of tidal disturbances or interactions with neighboring galaxies are observed, although there is a very slight disturbance to the right of the galaxy, possibly due to a small interaction. Overall, the galaxy seems to be a relatively undisturbed system undergoing only low levels of star formation.
