The galaxy presents a morphology consistent with an elliptical galaxy. It exhibits a smooth, centrally concentrated light profile, with the highest intensity near the core gradually diminishing outward. The overall shape appears somewhat elongated with an axis ratio of approximately 0.77. The galaxy's color is predominantly yellow-orange, suggesting an older stellar population with relatively low levels of recent star formation. There is little evidence of spiral arms or prominent dust lanes. Marginal irregularities exist, possibly indicative of minor gravitational interactions. The galaxy seems to have undergone minimal disturbances.
