The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution is dominated by a yellow-orange hue in the central region, suggesting an older stellar population. Fainter, diffuse blue light is subtly visible extending outward from the central bulge, perhaps indicative of ongoing, though subdued, star formation in the outer regions. The galaxy appears largely elliptical in shape, tending towards a rounded profile. There is no discernible spiral arm structure or bar. A subtle asymmetry or minor disturbance is suggested by slightly uneven light distribution on one side. Overall, the galaxy appears relatively isolated.
