The galaxy appears as a centrally concentrated object with a smooth luminosity profile, suggesting an elliptical morphology. The core region exhibits a bright, relatively homogenous emission signature. The overall shape is nearly circular, with a slight elongation that may indicate a very weak bar structure or a mild tidal interaction. There are subtle color gradients, transitioning from a slightly bluer hue in the central region to a redder component towards the outer halo. No distinct spiral arms or dust lanes are clearly visible. The smooth appearance suggests a lack of significant ongoing star formation activity. There is some indication of a very minor disturbance in the galaxy shape but that is difficult to see.
