This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a prominent central bulge that dominates its overall luminosity. The galaxy has an elongated shape, with its longest axis extending horizontally in the image. The color profile suggests an older stellar population, with a yellowish-orange hue concentrated in the central regions. There is a subtle color gradient, with the outer regions exhibiting a bluer tint, potentially indicating the presence of younger, bluer stars, though they are not particularly pronounced. There are no apparent spiral arms or distinct dust lanes. The overall structure suggests a galaxy that has undergone significant merging in its past, resulting in a well-mixed and relatively homogeneous stellar distribution. There's a slight irregularity or warp on the left side of the galaxy, which could indicate a minor gravitational disturbance or tidal interaction. The galaxy appears to be relatively isolated, with no obvious signs of major ongoing interactions.
