This galaxy appears to be an elliptical galaxy, with a smooth, diffuse light distribution. The central region exhibits a high surface brightness, appearing almost uniformly bright across the core, with no clearly defined nucleus. The overall shape is elongated, appearing cigar-shaped and indicative of a significant ellipticity, possibly an E5 or E6 on the Hubble classification scheme. There are no discernible spiral arms or dust lanes evident within this galaxy. The color is relatively uniform across the galaxy, with no strong gradients suggesting variations in stellar populations or ongoing star formation. The smooth light profile suggests that the galaxy is likely composed predominantly of older stellar populations, and that little to no major merger or star formation events have occurred in relatively recent times. There is no apparent evidence of tidal tails or other morphological features suggesting recent interactions with another galaxy.
