The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a centrally concentrated bulge that transitions into a more diffuse halo. There are some indications of bluer colored regions which suggests some star formation, but overall it appears to be mostly composed of older stellar populations. The galaxy displays no obvious spiral arm structures, major distortions, or tidal features, suggesting it has not undergone a recent major merger event, but some minor disturbances might be present. Its shape is approximately round, with a slight deviation toward a more intermediate form. There is a strong central concentration of light, possibly indicating an active galactic nucleus or a dense stellar core. Overall, the galaxy presents as a fairly well-formed system with moderate star formation.
