The observed galaxy presents an elliptical morphology, although some disk-like structure cannot be ruled out. The central region exhibits a high degree of luminosity, appearing almost uniform in brightness. Moving outward from the center, the luminosity decreases, displaying a smooth, gradual decline, which could indicate an extensive stellar halo or a diffuse distribution of older stars. The overall color appears to be reddish, suggesting an older stellar population and a relatively low rate of recent star formation. There are suggestions of tidal disturbances and what might be a merger event. The galaxy may be in the process of merging with a smaller galaxy.
