The galaxy presents as a relatively compact object, exhibiting a shape that deviates from a perfect ellipse. The overall appearance is characterized by a smooth distribution of light, suggesting it is likely an early-type galaxy. However, there is a possible indication of minor morphological disturbance. The colors indicate the presence of a diverse stellar population, with a dominant older population contributing redder hues. The light is centrally concentrated, which is consistent with an elliptical or lenticular morphology. The edges of the galaxy's light distribution are somewhat fuzzy, indicating a gradual decline in stellar density as one moves outward from the galaxy's core.
