The galaxy presents a generally smooth and elliptical morphology, lacking any prominent spiral arms or disk structures. It appears largely spheroidal, with a noticeable central bulge that dominates the overall light distribution. The galaxy exhibits a color gradient, with a more yellowish hue concentrated in the central regions, transitioning to a slightly bluer color towards the outer edges. This suggests a centrally concentrated population of older stars with lower ongoing star formation rates in the core, versus a more recent and ongoing formation of stars in its outer regions. The galaxy lacks any obvious signs of major disturbances or ongoing merger activity, such as tidal tails or irregular shapes. Overall, the galaxy appears to be a relatively quiescent system, potentially in a later stage of its evolution.
