The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. The luminosity profile appears to be dominated by an older stellar population, evidenced by the redder color index. There is a subtle indication of a disk, although no spiral arm structure can be determined from the image. The isophotes of the galaxy are elongated, suggesting a non-spherical shape, transitioning from a bright, unresolved core outward into a diffuse halo. There's a hint of disturbed morphology, but it is likely due to noise. Overall the galaxy does not show evidence of ongoing major merging activity or significant star formation.
