The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile.  The core region is a bright yellow-white, suggesting an older stellar population. Moving outward from the core, the color transitions to a more reddish hue, though the overall color remains relatively uniform throughout the galaxy's visible extent. There is little evidence of spiral arm structure or significant dust lanes. The galaxy has a moderate degree of ellipticity, being somewhat elongated. No obvious signs of active galactic nuclei features or strong star formation regions are readily apparent in this image. The overall morphology suggests a relatively evolved system with a dominant population of older stars.
