The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution. There appears to be an active galactic nucleus (AGN) or significant central concentration of light, with two bright central components. The overall color appears somewhat redder, suggesting an older stellar population. The light distribution indicates a relatively high degree of symmetry. There is no clear evidence of spiral arms or significant dust lanes. Based on the observed features, the galaxy is likely undergoing a significant merging event, perhaps nearing completion. There are some suggestions of minor disturbances to the galaxy's smooth form, but without further data it is difficult to determine the precise nature of the interaction.
