The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated luminosity gradient, appearing bright and slightly yellow, suggesting an older stellar population. There is a subtle transition in color towards the outer regions of the galaxy, exhibiting a hint of bluer tones possibly indicating younger stars. Faint extensions are visible. These may be tidal in nature, but the low signal to noise makes it difficult to be certain. The overall light distribution is consistent with an elliptical or lenticular galaxy, without prominent spiral arm structures. There are no distinct dust lanes or other features associated with active star formation.
