The galaxy presents a generally smooth, elliptical morphology. The central region displays a concentrated and bright luminosity profile, indicating a likely substantial stellar population. Moving outwards, the galaxy's light gradually diminishes, fading into the background sky. There are no clear signs of spiral arms or significant dust lanes, instead, there is a more homogenous texture, with a round appearance. Minor irregularities are observed in the outer regions that could be the result of a possible disturbance or ongoing interaction with a smaller galaxy. Overall, the image suggests a relatively evolved system.
