The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and centrally concentrated light distribution. It has an elongated shape, appearing more 'in between' round and cigar shaped than completely spherical. The central region exhibits a brighter, more intense luminosity, suggesting a higher concentration of stars towards the galactic nucleus. There is very little evidence of distinct spiral arms or significant dust lanes. The galaxy seems largely undisturbed, showing no major signs of ongoing or recent merger events. There might be minor distortions present, but they do not dominate the overall morphology.
