The galaxy presents as a slightly elongated, relatively smooth structure. A bright central bulge dominates the morphology, exhibiting a yellowish hue. This suggests an older stellar population concentrated towards the galaxy's center. Extending outwards from the central bulge is a faint, diffuse disk. There is some hint of bluer regions mixed in with the yellow, but they are not sharply defined. The shallowness of the blues could indicate areas of active star formation, though the general smoothness suggests a relatively low star formation rate overall. The galaxy appears largely undisturbed, showing no significant signs of major mergers or tidal interactions with other galaxies. There may be some minor disturbance visible. 
