The galaxy exhibits an elliptical morphology, appearing as a moderately flattened spheroid of light. The light distribution increases towards the center, which presents a bright, concentrated core region. The galaxy's color profile appears somewhat blueish, suggestive of ongoing star formation. The outer regions display a fainter, more diffuse glow. There is no obvious presence of spiral arms or a prominent disk structure. Some minor irregularities or disturbances could be present, suggesting the possibility of past or ongoing interactions.
