This galaxy appears to be a relatively undisturbed system, likely an elliptical or lenticular type. The light is concentrated towards the center, exhibiting a smooth, centrally condensed morphology. It possesses a bright, yellowish core, which suggests an older stellar population dominating the central region. Moving outward from the core, the light gradually fades, transitioning to a slightly bluer hue in the outer regions. This bluer color suggests the presence of a younger stellar population at larger radii, but it is not distinctly pronounced. The overall shape is moderately elongated. There is no clear evidence of spiral arms or significant dust lanes. No signs of a recent or ongoing major merger are readily apparent. Faint tidal features or minor disturbances may be present upon closer examination. The galaxy exhibits a measurable redshift, indicating its recession velocity and distance.
