The galaxy presents a somewhat lenticular morphology, with a noticeable central bulge. The light emanating from the bulge appears more yellow, suggesting an older stellar population and a lower rate of star formation. A faint disk extends outward from the bulge, exhibiting a bluer hue. The blue color indicates the presence of younger, hotter stars and ongoing star formation, although the disk appears relatively smooth, with no prominent spiral arm structure readily visible. The galaxy has a relatively compact size and appears to be a field galaxy. Overall, the galaxy's light profile indicates an intermediate mass system with signs of both old and more recent star formation activity. There are no signs of any major mergers. Some minor disturbance within the galaxy may be present, but it is difficult to confirm.
