This galaxy presents a largely smooth, elliptical morphology. The galaxy's light profile suggests a high degree of radial symmetry with no apparent spiral arm structure or significant disk component. It possesses a concentrated core, exhibiting a bright central bulge that fades into a more diffuse halo. There is a slight elongation, though the object appears very rounded overall. Color gradients are subtle, with a slightly redder hue concentrated toward the core region, potentially indicating an older stellar population in the center. There's some evidence of faint, bluer light in the outer regions of the galaxy, suggesting the presence of some younger stars, though the rate of star formation appears low overall. No obvious signs of tidal disturbances or recent merger activity are visible. 
