The galaxy presents as an elliptical morphology, exhibiting a predominantly smooth light distribution without any prominent spiral arms or disk-like features. Its shape appears somewhat elongated, falling between a perfectly round and cigar-shaped form. The central region of the galaxy appears to be the most luminous, with a gradual decrease in brightness toward the outer regions. The galaxy displays a yellowish-orange hue at the center. The outer regions are a bit more diffuse, and appear slightly more green. There is no evidence of strong tidal distortions or major merger events in the immediate vicinity, although there may be a slight asymmetry or minor disturbance present in the overall structure. The smooth appearance suggests a relatively passive galaxy with a population dominated by older stars. Overall, it appears as a high-mass galaxy with a relatively low star formation rate.
