The galaxy presents a flattened, elliptical morphology. It appears largely smooth in texture with a concentrated central bulge. The galaxy exhibits a yellowish-orange hue across the majority of its visible structure, with a slightly redder tint visible on one side of the galaxy. There is little evidence of significant spiral arm structures or prominent dust lanes. The smoothness and color profile suggest a galaxy dominated by an older stellar population, with suppressed rates of star formation. Its general form implies it is likely an elliptical galaxy, with moderate flattening. There is no strong visual indication of a major ongoing merger or tidal disturbance. A slight asymmetry is observed in the outer regions, however, these regions may contain disturbances.
