The galaxy appears to be a lenticular or early-type spiral galaxy, characterized by a smooth, centrally concentrated bulge and a faint, diffuse disk. The bulge dominates the overall luminosity, exhibiting an elliptical shape with a high degree of roundness. There is some indication of faint, disturbed features, possibly tidal arms or remnants of a minor merger, emanating from one side of the main body. The galaxy lacks prominent spiral arms. Color gradients suggest an older stellar population, particularly in the bulge, with a likely suppression of star formation across the galaxy.
