The galaxy presents a generally smooth, elliptical morphology. The primary component is a large spheroidal bulge, exhibiting a concentrated light profile, appearing quite round. The core region displays a yellow-orange hue, suggesting a population of older, redder stars. Fainter blue-ish regions are present on one side of the galaxy, possibly suggesting some level of recent star formation activity there. There is a suggestion of tidal disturbances or an ongoing merger due to its asymmetrical shape. Overall, the galaxy does not appear to have well-defined spiral arms or a prominent disk structure.
