The galaxy appears to be a relatively compact system with a smooth, elliptical morphology. The light distribution is concentrated towards the center, suggesting a high central stellar density. There appears to be a slight extension in one direction, perhaps indicative of a minor tidal disturbance or interaction, but the overall structure is dominated by a central bulge. The galaxy exhibits a color gradient, transitioning from a more reddish hue towards the core to a slightly bluer color in the outer regions. This could indicate a mix of older stellar populations in the center with a younger, more actively star-forming population in the outskirts, though star formation properties are not distinct. Despite the general smoothness, some faint irregularities are visible which suggest a slight interaction or possible merging of another galaxy in the system.
