The galaxy appears as a somewhat elongated, elliptical structure. Its light profile is relatively smooth, exhibiting a concentrated central region that gradually fades towards the outer edges. The color distribution across the galaxy suggests a mix of stellar populations. The central region exhibits a yellow-orange hue, indicative of older, cooler stars. A faint blue tinge is visible in the surrounding regions, suggesting the presence of some younger, hotter stars, although not in significant quantities. There is no strong evidence of spiral arms or other distinct features typically associated with disk galaxies. The galaxy does not show any obvious signs of major mergers or tidal disturbances, although subtle irregularities could indicate minor past interactions. The overall morphology is consistent with an elliptical galaxy that may be experiencing low levels of star formation.
