This galaxy exhibits a generally smooth morphology, with a high likelihood of being an elliptical or lenticular galaxy. The light distribution appears relatively even across the galaxy, with a slight color variation between the core and outer regions. The core appears to be more yellow-white, suggesting older stellar populations, while the outer edges may exhibit a slightly bluer hue, indicating the presence of some younger stars or star formation regions, although these are not very obvious. The galaxy is observed to be a slightly elongated shape, but is close to being round. There is little evidence of any spiral arm structure or significant dust lanes. The galaxy shows a fairly uniform appearance, with no signs of a recent major merger. However, there is a very slight asymmetry to the galaxy, which may be due to a minor disturbance or interaction with another object. It appears to be a massive galaxy, based on its luminosity and general appearance, and it is likely to have a low star formation rate.
