The galaxy presents as a concentrated, primarily smooth structure. The light profile is centrally concentrated, appearing roughly elliptical. A slight golden hue predominates in the core, gradually fading to a less saturated color with increasing radius. No distinct spiral arms or bar features are discernible. There is no evidence of strong dust lanes or recent merger activity, with only subtle asymmetries in its overall shape. The morphology appears generally regular and undisturbed. The galaxy’s light appears relatively uniform, lacking distinct bright knots or regions that would suggest recent star formation. The overall impression is of an evolved system, possibly an elliptical galaxy or a lenticular galaxy with a dominant bulge.
