The galaxy presents as a relatively smooth and centrally concentrated object. Its overall shape appears generally elliptical, exhibiting a gradual decline in luminosity from a bright, compact core outward. The central region displays a bright, whitish glow, suggesting a high density of stars. Moving outward from the core, the galaxy transitions into a bluer, more diffuse region with a hint of spiral arm structure. The arms are not well-defined, exhibiting a flocculent appearance. There is no clear indication of a distinct dust lane or strong star formation regions. Overall, the galaxy is intermediate in roundness with no major disturbances, and the galaxy appears to be isolated. The color gradient suggests a change in stellar population with older, redder stars concentrated in the center, and younger, bluer stars distributed in the outer regions.
