The galaxy presents as a relatively smooth, elliptical morphology. There is a general concentration of light towards the center, with a gradual decrease in luminosity towards the outer regions. The galaxy appears somewhat elongated, showing deviation from a perfectly circular shape. Color gradients suggest a central region that is redder in color, indicating an older stellar population and a relative paucity of ongoing star formation in the core. There are no clearly defined spiral arms or prominent dust lanes visible. There is a very slight asymmetry in its structure, which could indicate some past or ongoing gravitational interaction, although this is not definitive.