The galaxy presents an elliptical morphology, exhibiting a smooth and diffuse light distribution. It is oriented roughly horizontally in the image, with a clear central bulge region that is slightly elongated. The color profile suggests a generally evolved stellar population, indicated by the reddish hues concentrated in the central bulge. Fainter, bluer regions are observed extending outwards from the bulge, possibly indicative of ongoing or recent star formation within the galaxy. There are indications of a faint disk-like structure. There appears to be a slight asymmetry in the outer regions of the galaxy. Overall, it has a relatively quiescent appearance, lacking any strong signs of active galactic nuclei or major disturbances.
