The galaxy presents as a slightly elongated, moderately concentrated object. Its color profile suggests a dominant older stellar population, appearing yellowish-orange in the composite image. The overall structure is relatively smooth with a high degree of central light concentration, showing minimal evidence of spiral arms or significant dust lanes. There is a subtle suggestion of an extended halo or outer region surrounding the brighter core. No signs of active galactic nuclei (AGN) or significant star formation regions are immediately apparent. There may be a tidal feature or minor interaction with another galaxy nearby, but evidence is not conclusive.
