The galaxy presents a primarily elliptical morphology. It appears as a smooth, centrally concentrated object, exhibiting a gradual decline in luminosity from the core outwards. The dominant color is yellowish-orange, suggesting an older stellar population and minimal ongoing star formation. There are some indications of bluer regions at the edges of the halo, which could be indicative of more recent star formation or scattering of blue light. There is no obvious dust lane or spiral arm structure, with the galaxy presenting a primarily homogenous appearance. There is no evidence of a major merger or significant tidal distortion in the immediate vicinity, though there is some asymmetry in the outer halo, suggesting a potential interaction. The galaxy is moderately luminous.
