The galaxy presents as having a relatively smooth morphology, with a dominant central bulge and a faint, ill-defined disk structure. The bulge exhibits a yellowish hue, potentially indicative of an older stellar population. A portion of the disk appears somewhat more orange in color, suggesting ongoing or recent star formation, although at a low rate. There appears to be minor disturbances from a possible merging event on the lower-right part of the galaxy. The galaxy is generally round in appearance.
