The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. There is a noticeable color gradient, trending from a yellowish-white core to a fainter, bluer outer region. The galaxy appears to be relatively isolated, with no immediate signs of major tidal disturbance or ongoing merger activity, although subtle minor disturbances cannot be ruled out. The shape of the galaxy is more in-between, more like a rounded disk than a perfect sphere or cigar shape. The galaxy's angular size is small, suggesting it is at a substantial distance. Based on its color profile, it's likely that the core is composed of older stellar populations while younger stars may be present in the surrounding disk.
