The galaxy exhibits a generally smooth morphology, with a dominant central bulge. The light distribution is relatively uniform across the bulge, although there is a slight increase in luminosity towards the center. I observe a distinct tidal tail emanating from the galaxy, suggesting a recent or ongoing interaction with another celestial object. Furthermore, there are signs of some morphological disturbance in the central region, possibly due to the interaction. The overall color of the galaxy is somewhat redder, which suggests an older stellar population and reduced star formation. The galaxy appears nearly circular, with a slight elongation that might be indicative of a disk component. However, the dominant feature is the smooth, elliptical appearance of the bulge.
