The galaxy presents an elliptical morphology, appearing elongated with a high axial ratio. The central region exhibits a bright, concentrated bulge, suggesting a high stellar density and potentially an older stellar population dominating. The color gradient moves from a yellowish-orange at the core, indicative of older, redder stars, to a bluer hue in the outer regions of the disk, possibly reflecting younger star formation activity. The disk is relatively smooth, lacking prominent spiral arms or distinct dust lanes, but may display some faint features. There is no obvious evidence of a major merger event. The galaxy is seen at an angle, the exact inclination cannot be determined without further analysis.
