The galaxy presents as a primarily smooth, disk-like structure with intermediate ellipticity. The central bulge exhibits a concentrated and bright yellowish-white glow. A faint disk surrounds the bulge, displaying a slightly bluer hue. There is a suggestion of some minor disturbance in the disk's morphology, as it is not perfectly uniform. However, there are no clear signs of ongoing major merging activity or tidal tails. The overall structure suggests a relatively evolved system with an estimated stellar mass greater than 10^11 solar masses and moderate star formation activity. The galaxy's light profile suggests an overall 'in between' rounded shape, not perfectly circular nor extremely elongated.
