The galaxy presents as a slightly elongated, smooth object, exhibiting a noticeable red-shifted color profile with a bright central concentration. Fainter, diffuse light extends from the central region along the major axis, fading into the background. Some evidence suggests the presence of a faint disk-like structure with a slight inclination relative to our line of sight. There appears to be a subtle asymmetry to the galaxy's outer regions, particularly on one side, which could indicate a minor gravitational disturbance or interaction. Overall, the galaxy appears to be a relatively massive system, with low star formation activity and an old stellar population dominating its light output.
