The galaxy presents a generally smooth morphology, appearing mostly rounded in shape. There is a suggestion of faint, diffuse features, possibly indicating a disk-like component, though the smoothness is dominant. The galaxy exhibits a color gradient, transitioning from a central yellowish-orange hue to a fainter, bluer periphery. This could indicate a change in stellar population, with the core potentially dominated by older, redder stars and the outer regions containing younger, bluer stars or ongoing star formation. There also appears to be some sort of minor disturbance and some sort of merging behavior, as the general shape is not perfectly symmetrical.
