The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile with a high degree of central luminosity. It presents a somewhat elongated shape, with a possible slight flattening. The galaxy's color suggests a relatively old stellar population, with a redder hue indicative of aging stars and lower ongoing star formation activity. No distinct spiral arm structures or dust lanes are visible. The overall morphology suggests a system that has undergone significant dynamical relaxation, possibly through mergers or interactions in its past. There is some asymmetry in the outer regions that could indicate a past or ongoing minor interaction.
