The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The core is a bright, concentrated region, appearing yellowish in color, potentially indicating an older stellar population. Moving outward from the core, the light gradually fades into the surrounding galactic halo. There is a hint of a reddish hue enveloping the galaxy, especially closer to the core, indicative of dust attenuation or the presence of older, redder stars. There's a slight elongation observed, deviating from a perfect circular shape, suggesting a non-zero ellipticity. No obvious spiral arms or distinct features like star-forming regions are discernible in this image, further supporting the classification as an elliptical galaxy. The overall impression is that of a mature, relatively quiescent system with a dominant bulge component.
