The galaxy presents as a centrally concentrated, elliptical structure. Its morphology appears smooth, lacking any distinct spiral arms or bar features. The light distribution shows a gradual decrease in intensity from the core towards the outer regions, suggesting an absence of significant recent star formation within the disk. There is an observed shift in color from the center out to the edge of the object, with the inner region having a more yellow/orange hue, and the outer region tending towards red. Given the smooth appearance and color gradients, this galaxy likely belongs to an earlier type classification. There is no visible evidence of tidal disturbances or ongoing merger activity; the galaxy appears to be relatively isolated and undisturbed.
