The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into a less defined outer region. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, potentially indicative of a lack of ongoing star formation there. The outer regions show a slight bluer tint, which could imply the presence of younger stars or regions of mild star formation, though these are not very prominent. There is a very small visual disturbance to the bottom left of the galaxy, but it does not seem to be significantly affecting the primary structure or morphology. Overall, the galaxy presents as a fairly regular, early-type system.
