The galaxy presents an overall smooth morphology. It has a slightly elliptical shape, appearing more elongated than perfectly circular.  The central region displays a concentrated brightness, suggesting a dense core.  Fainter light extends outward from the center, contributing to a diffuse halo surrounding the galaxy. There is a subtle asymmetry in the outer regions, hinting at a possible minor disturbance or interaction. There is also a faint, blue tinge near the center and in small areas outside the core, suggesting a small amount of star formation may be occurring. Overall, the galaxy appears to be a relatively massive system, with a modest rate of star formation. There do not seem to be any prominent spiral arms or obvious signs of a major ongoing merger.
