The galaxy presents an elliptical morphology, exhibiting a smooth, relatively featureless structure. It is centrally concentrated with a gradual decrease in luminosity outward. The color profile suggests an older stellar population, appearing generally reddish-yellow. There is a slight hint of asymmetry, potentially indicating a minor gravitational interaction or disturbance in its recent history. No obvious spiral arms or dust lanes are discernible. The galaxy appears to be relatively isolated within its immediate environment, with no clear signs of ongoing major mergers.
