The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, appearing yellowish, suggesting a population of older stars. There is a slight elongation in the morphology, deviating from a perfectly circular shape. Faint extensions or tidal features are potentially present. A subtle color gradient seems apparent, with the outer regions displaying a hint of bluer hues, possibly indicating areas of recent, albeit minimal, star formation activity. There is no clear indication of spiral arms or a well-defined disk structure. Overall, the galaxy appears as a system with a dominant bulge and a smoothly distributed stellar population. There is a subtle disturbance potentially indicating a minor interaction with another galaxy or past merger event.
