The galaxy presents as a moderately bright elliptical system, exhibiting a smooth, featureless morphology. The core region is characterized by a concentrated luminosity, displaying a yellowish-white hue, suggestive of an older stellar population. The light gradually diminishes toward the outer edges. The galaxy shows an elongated shape, being neither perfectly spherical nor highly flattened. There is a very slight suggestion of some tidal disturbance. The absence of distinct spiral arms or prominent dust lanes reinforces its classification as an elliptical galaxy, where star formation is likely suppressed.