The galaxy presents as a lenticular-type, displaying a smooth, relatively featureless disk component. A subtle central bulge is visible, with a slightly enhanced yellowish color, indicating a population of older stars in this region. The disk itself exhibits a bluer hue, suggesting the presence of younger stars. The overall structure is somewhat disturbed, showing signs of possible minor interaction. There is no distinct spiral structure, suggesting a more evolved morphology. No strong active galactic nuclei activity is apparent from the image. The galaxy appears to be relatively isolated.
