The galaxy presents as a relatively smooth, elliptical morphology. A dominant central bulge of concentrated luminosity suggests an older stellar population. There is a slight elongation but is mostly rounded. The central region exhibits a bright, yellowish-orange hue, potentially indicating the presence of evolved stars. Faint, diffuse extensions are visible, but no distinct spiral arms or significant dust lanes are discernible. There may be a minor disturbance or possible interaction with a neighboring object to the upper right but it cannot be stated definitively. The overall structure appears relaxed and stable.