The galaxy appears to be a relatively smooth, somewhat elliptical system. It exhibits a concentrated central bulge region that appears yellowish-orange in color. This coloration may indicate an older stellar population with relatively low ongoing star formation. There is a faint disk component visible but it has no visible spiral arms. The disk fades into the background at a relatively short distance. There are no significant signs of mergers or tidal disturbances, though very minor disturbances cannot be ruled out. The overall morphology suggests a galaxy that is undergoing a transition, potentially evolving from a spiral to a more elliptical form.
