The galaxy presents as an elliptical morphology, characterized by a smooth, relatively featureless structure. Its overall shape appears predominantly round, displaying minimal deviation from circular symmetry. There are no visible spiral arms, bars, or significant dust lanes. The light distribution across the galaxy is concentrated toward the center, suggesting a dense galactic nucleus, with luminosity gradually decreasing towards the outer edges. Coloration is predominantly yellow, indicating an older stellar population. The lack of blue hues suggests a low rate of ongoing star formation. There is no evidence of any major merger events, and the galaxy is undisturbed.
