The galaxy appears to be of an elliptical morphology, displaying a smooth and centrally concentrated luminosity profile. The overall shape is elongated, deviating significantly from a circular form.  The color gradients suggest an older stellar population, indicated by the reddish hue concentrated in the central bulge region. A faint, diffuse halo surrounds the galaxy, exhibiting a lower surface brightness than the central bulge. The galaxy may be in the process of merging with another, smaller galaxy, or experiencing minor tidal disturbances that do not significantly disrupt its overall structure. The luminosity is consistent with a high redshift object. 
