The galaxy presents as a relatively smooth, elliptical-like structure. It has a concentrated central bulge that appears a yellowish hue, suggesting an older stellar population dominates this region. The color becomes slightly bluer towards the outer regions indicating the presence of younger stars. There is little to no visible spiral arm structure or prominent dust lanes, further supporting the classification of a relatively evolved galaxy. It appears fairly undisturbed, without significant signs of ongoing major mergers or tidal interactions with other galaxies, only minor disturbances. The galaxy appears nearly circular, with no extreme elongation or asymmetry. There is no distinct nucleus, the luminosity gradually increases to a bright center. 
