The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears roughly spheroidal. The outer regions of the galaxy gradually fade, lacking sharply defined edges. There is some indication of a very faint disk-like structure, but it is not clearly delineated. No significant signs of tidal disturbances or merging events are readily apparent. The color profile suggests a population of older stars, with a dominant yellowish hue, especially in the central region. There appears to be little active star formation evident in this image. Overall, the galaxy appears to be a relatively quiescent system, with a substantial stellar mass and a low star formation rate.