The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its light profile suggests minimal or no discernible spiral arm structure. The galaxy's overall color is moderately red, hinting at a predominantly older stellar population with relatively low ongoing star formation. The axial ratio of the galaxy is close to one suggesting that the system is close to face-on. The galaxy appears to be relatively isolated, with no obvious signs of major gravitational interaction or tidal disturbance in its immediate vicinity. There are no pronounced dust lanes or prominent HII regions visible within the galaxy.
