The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a high degree of light concentration. There is evidence of disk-like structure, which could also be evidence of a recent merger or tidal interaction. The galaxy displays a color gradient, transitioning from bluer hues in its outer regions to redder tones towards its central bulge. This indicates a potential variation in stellar populations, with older, redder stars likely dominating the core and younger, bluer stars residing in the disk-like regions. The overall luminosity suggests a relatively massive system, with moderate ongoing star formation.
