This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color gradient shifts from a yellowish hue in the core to a slightly bluer tint in the outer regions. The morphology suggests a system dominated by older stellar populations, though some ongoing or recent star formation activity might be present, suggested by the blue-ish tint. There are no obvious signs of spiral arms, strong dust lanes, or tidal disturbances. Overall, the galaxy appears to be a generally undisturbed, relatively evolved system. The elongation implies it's not perfectly spherical, leaning towards a slightly cigar-like shape. There is no obvious evidence of a major merger or significant interaction with other galaxies.
