The galaxy presents as an elliptical-like morphology, appearing smooth and relatively featureless in the available image. Its shape is moderately elongated, but deviates slightly from being perfectly spherical, suggesting a slight degree of flattening. The central region exhibits a higher surface brightness, indicative of a concentrated stellar population. The galaxy displays a yellowish-red color profile which suggests an older stellar population, potentially indicating a low rate of on-going star formation. There is little evidence of spiral arms or dust lanes. There might be evidence of a minor disturbance, but this is difficult to assess with certainty given the image quality.
