The galaxy presents an overall elliptical morphology, with a smooth appearance and a high degree of central concentration of light. It displays a yellow-orange hue, indicative of an older stellar population with fewer hot, young stars and more evolved red giants. The galaxy's shape is elongated, leaning towards a cigar-like morphology.

There is a slight hint of possible tidal disturbances or faint extensions of material emanating from one end of the galaxy, potentially suggesting minor gravitational interactions. The galaxy seems relatively isolated in its immediate environment, without evidence of a major ongoing merger or interaction with another galaxy.
