This galaxy presents as a somewhat elliptical, relatively smooth structure. The central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar density or potentially an active galactic nucleus. The isophotes appear moderately flattened, displaying a noticeable deviation from a perfectly circular shape.

There is a subtle color gradient observed, transitioning from a bluer hue in the central area to slightly redder tones in the outer regions. This could suggest varying stellar populations or dust content across the galaxy. No distinct spiral arms or prominent dust lanes are visible. There might be a very subtle degree of disturbance in its form but it does not appear to be undergoing a major merger or significant interaction with another galaxy.
