The galaxy presents as a relatively smooth, centrally concentrated object with a slight ellipticity. The core region appears to be dominated by older stellar populations, exhibiting a yellowish-red hue. Fainter, bluer light extends outward from the central bulge, suggesting the presence of some younger stars or ongoing star formation within the galaxy's disk. There is a hint of a possible disk structure, but no distinct spiral arms are discernible. There is no strong evidence of major morphological disturbances or ongoing merger activity. Faint color variations exist within the outer regions of the galaxy, but generally speaking the color is uniform. 
