The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a moderately smooth, elliptical light distribution. It is slightly elongated, but generally rounded in shape. The color gradient suggests a predominantly older stellar population, concentrated toward the center, with a yellowish hue indicative of evolved stars. There is very little evidence of spiral arm structure or active star formation, although a small amount of bluer light is observed on the edges of the galaxy. There are some minor indications of disturbance or interaction, but no major signs of tidal tails or ongoing merger events.
