The galaxy presents as a somewhat elliptical, disk-like structure with a smooth texture. The central region is characterized by a bright, concentrated bulge, exhibiting a yellowish hue, which suggests an older stellar population. Moving outwards from the center, the light gradually diminishes, and the overall color shifts subtly towards redder tones, although it's very subtle. There appear to be minor disturbances in its form, but they are difficult to discern with certainty. No distinct spiral arms or prominent dust lanes are visible. Overall, the morphology suggests an intermediate galaxy between a pure elliptical and a spiral, possibly an S0 or early-type spiral with a dominant bulge.
