The galaxy presents as a single, relatively smooth object with a concentrated central bulge exhibiting a yellowish-orange hue. There's a slight extension of light surrounding the core, transitioning into a fainter, more diffuse halo. The object's shape is generally elliptical, appearing mostly round but with a slight elongation. There are no distinct spiral arms or dust lanes visible. The overall structure suggests a system dominated by an older stellar population, with little evidence of ongoing major star formation or recent merger activity. The light distribution indicates a fairly evolved system with a high degree of central concentration.
