The galaxy appears to be an early-type system, likely an elliptical or lenticular galaxy, characterized by a smooth and relatively featureless morphology. It exhibits a concentrated, centrally bright bulge region, which contributes significantly to its overall luminosity. The galaxy displays a yellowish-red hue, indicative of an older stellar population with suppressed star formation. There may be ongoing or recent merger activity present, as there are visual disturbances of some kind. The overall shape appears mostly round.
