The galaxy appears to be a relatively bright, early-type system, possibly an elliptical or lenticular galaxy. Its overall shape is somewhat elongated but generally smooth, with the bulk of its light concentrated in a central bulge region. The color profile indicates an older stellar population, with a yellowish-orange hue dominating the galaxy's appearance. This suggests a lower rate of ongoing star formation compared to late-type spiral galaxies. There is a slight asymmetry visible, perhaps an indicator of a past or ongoing minor interaction. The disk appears diffuse. The galaxy is fairly isolated.
