The galaxy presents a generally elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant stellar population density and possibly an active galactic nucleus. The surrounding halo shows a gradual decrease in light intensity, appearing relatively smooth with no prominent spiral arm structures or dust lanes visible. Faint, diffuse extensions are present along one side of the galaxy, possibly indicating tidal interactions or past merger events, though no major disturbance is immediately evident in the galaxy's overall form. The color indices indicate a redder overall color, suggesting an older stellar population with relatively low current star formation activity. There is also indication of a bluer, star-forming region present in the image off center from the main galaxy.
