The galaxy appears as a relatively compact object, exhibiting a predominantly smooth morphology. It is generally elliptical in shape, appearing subtly elongated rather than perfectly spherical. The central region displays a brighter, more concentrated luminosity, suggesting a significant stellar density or possibly an active galactic nucleus. The galaxy's color profile indicates a higher concentration of older stellar populations. While the overall structure appears largely undisturbed, there is a faint indication of possible minor tidal interactions. Based on its observed characteristics, it is likely a massive elliptical galaxy with a low ongoing star formation rate.
