The galaxy presents a smooth, elliptical morphology. It appears elongated, with an approximate aspect ratio suggesting a cigar-like shape. There is no obvious evidence of a spiral arm structure or significant dust lanes. The light distribution is concentrated towards the center, with a diffuse halo surrounding the core. Color gradients are subtle, with a slight bluish tint observed in the outer regions, transitioning to a redder hue towards the nucleus. No major or minor disturbances are apparent, and the galaxy appears to be relatively isolated, showing no indications of a recent or ongoing merger event.
