The galaxy presents as a slightly elongated, lenticular-shaped object with a smooth and diffuse appearance. The central region exhibits a higher concentration of light, appearing brighter and more yellowish in color, indicative of an older stellar population. Fainter, bluer light is visible in the outer regions, suggesting more recent star formation, though this is less prominent. There is no clear spiral arm structure or distinct dust lanes visible. Overall, the galaxy appears relatively undisturbed, without significant signs of ongoing major mergers or tidal interactions. The color gradients suggest a degree of stellar population segregation, with older, redder stars concentrated in the bulge, and younger, bluer stars in the outer disk.
