The object appears to be a relatively small, low-mass galaxy. It displays a generally amorphous morphology with a diffuse, faint glow. There are no distinct spiral arms or a well-defined central bulge evident. The light distribution suggests a relatively smooth structure overall, though some subtle irregularities hint at possible disturbances. There is a bluer hue toward the center, possibly indicating a region of more active, albeit low-level, star formation there. The surrounding area appears relatively devoid of distinct structures or features, implying it is not actively interacting with any larger galaxies in close proximity, though evidence of a recent minor merger is not ruled out.
