The object presents as a galaxy, exhibiting an elliptical morphology with a relatively smooth texture. The color profile suggests a redder hue, implying an older stellar population. The shape appears largely round with a slight deviation towards an intermediate form. Evidence suggests the object might be undergoing an interaction, or a merger event, that presents with the potential of some minor disturbances. Overall, the galaxy appears primarily smooth with traces of internal structures that may or may not be signs of disturbance.
