The galaxy presents a somewhat smooth morphology, exhibiting an elliptical shape. It is primarily characterized by a concentrated central bulge, indicated by a bright and nearly circular core. There is some evidence of disk structure as well, but no clear spiral arms are observed. Faint outer regions extend beyond the core. The overall color suggests an older stellar population with relatively low levels of ongoing star formation. There may be evidence of minor disturbances to its structure, perhaps indicating interactions with a smaller object, or an earlier merger event. There is no clearly defined tidal tail. It may be involved in a merger or may be interacting with another galaxy that is out of frame.
