The galaxy presents as a relatively smooth, elliptical-like structure. It has a moderately compact core region surrounded by a more diffuse halo. One side of the galaxy appears more elongated or extended than the other, but no distinct spiral arms or well-defined features are discernible. The color gradient suggests a possible difference in stellar populations, with a central region exhibiting bluer tones which may indicate a greater presence of younger, hotter stars or ongoing star formation, while the outskirts appear redder, possibly indicating an older stellar population. A notable feature is a distinct redder patch on one side of the main galactic body, possibly a region of dust obscuration, or a separate, smaller galaxy undergoing a minor merger. Overall, the galaxy's morphology suggests it may be in a relatively late stage of its evolution.
