This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. There is little evidence of spiral arms or significant dust lanes. It shows a slightly elongated shape, somewhere between rounded and cigar shaped. The galaxy presents a blue hue, suggesting the presence of at least some relatively young stars. The lack of significant distortions suggests that it is not currently undergoing a major merger, although there is a minor disturbance. I estimate the galaxy's diameter to be around 7 kpc based on the provided information. The galaxy has an estimated stellar mass of approximately 10^10.3 solar masses and exhibits signs of ongoing star formation.
