The galaxy presents an elliptical morphology, elongated with an axial ratio of approximately 0.6. The galaxy has a smooth, diffuse appearance indicating it may be an elliptical galaxy. There appears to be a central bulge that is distinctively brighter than the surrounding halo. The color gradient of the galaxy appears to shift from a yellow hue towards the center, suggestive of an older stellar population. Towards the outer regions of the galaxy, the color turns to more blue, indicating the presence of younger stars. This galaxy is likely 5.7 kpc in radius. The overall light distribution follows a relatively simple Sersic profile. There is some sign of tidal disturbance.
