The galaxy appears to be an elliptical galaxy, exhibiting a smooth, nearly spheroidal morphology. The central region presents a concentrated and bright luminosity, indicative of a dense stellar population. The light gradually fades towards the outer regions. The galaxy shows a slightly elongated shape. Overall, there isn't any obvious evidence of spiral arms or significant dust lanes in this image. The color gradient shifts subtly from a yellowish-white at the core, transitioning to a slightly bluer hue in the outer edges. This suggests a potential radial variation in stellar population, with older, redder stars concentrated centrally and a presence of younger, bluer stars within the galaxy.
