The galaxy presents a generally elliptical morphology, with a smooth, concentrated central bulge exhibiting a reddish hue. This suggests a dominant population of older, redder stars within the bulge. The outer regions of the galaxy appear more diffuse and display a bluer color, potentially indicating ongoing or recent star formation within a disk component. While the overall structure is smooth, there are hints of subtle asymmetries or disturbances in the outer regions, though not definitively indicative of a major merger. The galaxy appears to be in a relatively quiescent state with modest star formation activity. Its elongated shape, which is neither perfectly round nor highly elongated, indicates it is somewhere in between the two.
