The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth light distribution. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the light gradually fades, transitioning into a more diffuse, blueish halo. There's a slight elongation, giving it a somewhat cigar-shaped appearance, but generally it seems fairly well-rounded. No prominent spiral arms or dust lanes are visible. There are no obvious signs of recent major merger activity or significant tidal disturbances based on the symmetry and light distribution of the galaxy. The galaxy seems to be a relatively quiescent system, possibly with a low rate of current star formation.
