The galaxy presents a primarily smooth morphology with a somewhat rounded shape. There is a hint of a disk-like structure but it is not prominent. The color gradient suggests an older stellar population. The central region appears more yellow, indicative of evolved stars, transitioning outwards to a slightly redder hue, which might suggest regions of dust obscuration or differing stellar populations. The overall structure appears relatively undisturbed, without obvious signs of a major merger or tidal interactions. However, a subtle asymmetry may indicate minor disturbances. The galaxy appears to be undergoing relatively low levels of star formation activity.
