The galaxy appears as a lenticular or possibly an early-type spiral galaxy, exhibiting a relatively smooth light distribution. The central bulge is prominent and appears quite bright and concentrated, with a yellowish-white color, indicative of an older stellar population. The disk component is fainter and bluer in color, suggesting ongoing star formation, albeit at a moderate rate. The spiral arms, if present, are not well-defined and appear tightly wound. The galaxy shows no major disturbances or signs of an ongoing major merger event, however a possible minor disturbance is present.
