The galaxy exhibits a relatively smooth morphology, with a dominant central bulge exhibiting a yellowish hue. A faint, disk-like structure surrounds the bulge, oriented approximately horizontally. The disk shows hints of blue, suggesting the presence of younger stellar populations and ongoing star formation. The galaxy appears to be somewhat elongated, but largely elliptical. There are only minor irregularities observed, with little evidence of ongoing major mergers or significant tidal disturbances. Overall, the galaxy appears to be an intermediate system, between a pure elliptical and a spiral galaxy.