The galaxy presents as a somewhat elongated, lenticular-like system, viewed at a considerable angle relative to its disk. A central, yellowish bulge dominates the galaxy's overall appearance, exhibiting a higher concentration of light and suggesting a population of older stars. Surrounding the bulge is a fainter, bluer disk component that appears relatively smooth with only subtle indications of spiral structure. The color gradient from the center outwards suggests ongoing, albeit moderate, star formation within the disk. There are no obvious signs of major merger events, though some minor tidal disturbances cannot be ruled out at this resolution. The galaxy's morphology leans towards being relatively smooth overall, rather than exhibiting strong, distinct features.
